The galaxy presents as an elliptical or lenticular form, although some structure suggesting a disk component is present. The light profile exhibits a concentrated, bright central bulge, transitioning outwards into a more diffuse halo. The color appears generally red, with a slightly bluer tint at the very edges, possibly indicating some ongoing star formation. There is no significant evidence of tidal tails or strong morphological disturbances indicative of a recent major merger. Faint structures and a dusty area are observable and may have resulted from a past minor merger. The overall morphology appears relatively smooth and settled.
