The galaxy presents a generally smooth and concentrated appearance, with an elliptical morphology. A bright, centralized core is evident, surrounded by a more diffuse halo of light. The overall color gradient suggests a population of older stars, with a yellowish hue dominating the central regions, potentially indicating a lack of significant ongoing star formation in the core. The outer regions display a slightly bluer tint, hinting at the presence of a younger stellar population. Subtle distortions or tidal features are not immediately apparent, suggesting a relatively relaxed dynamical state. There is no clear indication of spiral arms or a distinct disk structure. The galaxy appears to be a fairly massive system based on its overall luminosity, with a modest rate of star formation.
