The galaxy presents as a lenticular-like system, exhibiting a smooth, centrally concentrated bulge with a surrounding, relatively featureless disk. The disk is oriented approximately edge-on with a position angle of roughly 149 degrees, as observed from our vantage point. The elliptical morphology is quite pronounced, suggesting a significant deviation from circularity in its overall shape. The central bulge appears yellowish-white, with a gradual decrease in surface brightness outwards. The relative colors indicate an older stellar population dominating the bulge. The disk component appears fainter and somewhat bluer in comparison to the bulge, potentially suggesting the presence of ongoing star formation or a younger stellar population in the outer regions. There is no apparent spiral arm structure discernable in this image. Minor dust lane features may be present, but this is difficult to confirm with the limited resolution. The system does not appear to be actively merging or interacting with another galaxy, and there is no obvious morphological evidence of recent major disturbances. Overall, the galaxy presents a moderately evolved morphology, possibly transitioning from a spiral to an elliptical system.
