The galaxy presents as a lenticular or possibly an elliptical galaxy, as its morphology is generally smooth with little discernible internal structure such as spiral arms. It exhibits a flattened, cigar-like shape, suggesting it is viewed close to edge-on. There is a central bulge that appears brighter and more concentrated, with the intensity diminishing gradually towards the outer edges. A slight color gradient is visible, with the central region exhibiting a redder hue, possibly indicating an older stellar population. Fainter, bluer regions appear towards the outer edges of the galaxy disk, potentially indicating some ongoing star formation. There are no obvious signs of a major merger or significant tidal disturbances; however, the slight asymmetry in the outer disk could be indicative of minor interaction or past merger events. Overall, the galaxy appears to be a relatively evolved system with a mixed population of stars and potentially moderate star formation in the outer regions.
