The galaxy presents as a primarily smooth, elliptical object. Its light is concentrated in the center, with a gradual decrease in luminosity moving outwards. The galaxy appears elongated, with an approximate ratio of 2:1 between its major and minor axes. There is no apparent evidence of spiral arm structure or significant dust lanes. The morphology is largely undisturbed, with no strong indications of ongoing or recent major merger activity. Faint color gradients may be present, with the central regions exhibiting a slightly yellower hue than the outer halo. Overall, the galaxy appears to be a relatively evolved system with a population of older stars.
