This galaxy appears to be a relatively smooth, elliptical or lenticular type, with a noticeable bulge. The central region exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. The outer regions show a gradual decrease in brightness, fading into a diffuse halo. The galaxy has an elongated shape, being more cigar-shaped than perfectly round. There is no apparent spiral structure or evidence of ongoing major mergers. The morphology indicates a system that is either a single, evolved galaxy or the result of a past merger that has reached a state of relative equilibrium.
