The galaxy presents as a somewhat elongated, lenticular-like structure. A dominant, smooth central bulge is observed with a yellowish-white hue, indicating a population of older stars. The outer regions exhibit a fainter, more diffuse disk component, with hints of bluer regions possibly indicating areas of ongoing star formation. There are also a few distinct reddish areas within the disk, perhaps representative of dust lanes or obscured HII regions. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event, though there are some hints of minor tidal disturbances around the structure. The overall morphology leans towards a generally round shape, but some elongation is present.
