The galaxy presents as a centrally concentrated, luminous object, with a generally smooth, elliptical morphology. A bright, prominent core dominates the visual structure, surrounded by a more diffuse halo of light. The color profile is generally yellowish-white, indicating a population of older stars. There is a suggestion of some bluer light extending towards the left side of the image, which could indicate a weak disk feature or ongoing star formation. There is no strong indication of spiral arm structure or significant dust lanes. The outer regions exhibit a gradual fading into the background sky, indicative of a lack of sharp boundaries or truncation of the stellar population. Possible minor disturbances or interactions may be subtly present.
