This galaxy presents as a fairly smooth and centrally concentrated structure. It exhibits an elliptical morphology, appearing somewhat flattened rather than perfectly spherical. The color profile suggests a dominant population of older stars, as indicated by the yellowish-red hue in the central region, which likely corresponds to a bulge. The outer regions appear slightly bluer, hinting at a small amount of ongoing star formation. No distinct spiral arms or strong dust lanes are visible. The galaxy seems relatively isolated, with no obvious signs of interaction or tidal disturbances. Overall, it appears to be a mature galaxy, possibly in transition from a spiral to an elliptical type.
