This galaxy presents as a relatively smooth, elliptical-like object. The light is concentrated towards the center, indicating a high central stellar density. There is a gradual decrease in luminosity moving outward from the core, with no discernible spiral arm structure or dust lanes. The overall color appears to be yellow and red, suggesting an older stellar population and a low star formation rate. There is no visual evidence of any recent or ongoing major merging events or significant tidal disturbances affecting the galaxy's morphology. The galaxy exhibits a high degree of rotational symmetry and can be characterized as nearly circular when viewed in projection, which can be an indication of it being an elliptical galaxy.
