The galaxy presents as a single, relatively smooth, and centrally concentrated object. Its morphology appears predominantly elliptical or spheroidal, with a high degree of central symmetry. The color profile indicates a strong concentration of light towards the center, gradually fading outwards. The central region appears yellowish, suggesting a population of older stars. The outer regions exhibit a slightly bluer hue, potentially indicating a younger stellar population or ongoing low-level star formation, though this activity is likely concentrated in the outer regions. There is no visible evidence of spiral arms or a distinct disk structure. No major disturbances or signs of recent merging events are evident, although minor tidal features cannot be completely ruled out at this resolution. The overall structure and color gradients suggest a mature galaxy, possibly undergoing passive evolution.
