The galaxy appears to be an elliptical galaxy, as indicated by its smooth, relatively featureless morphology. It exhibits a concentrated, bright central region, suggesting a high density of stars within the core. The galaxy's overall shape is elongated, resembling a prolate spheroid. It displays a smooth, diffuse halo surrounding the central bulge, with a gradual decline in brightness towards the outer edges. There is a subtle color gradient visible, with the central regions exhibiting a yellowish or golden hue, potentially indicating an older stellar population, while the outer regions appear slightly bluer, suggesting the presence of a younger stellar population and ongoing star formation. There is no clear evidence of spiral arms, dust lanes, or any significant disturbances in its morphology. It does not appear to be undergoing any major merging events, though there may be minor gravitational interactions with smaller objects or evidence of a past merger.
