The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slight ellipticity, appearing more "in-between" round and elongated rather than perfectly spherical. The central region displays a bright, concentrated luminosity, suggesting a significant stellar population and/or active galactic nucleus. Extending outward from the core, there's a more diffuse halo with a fainter, bluer color. I do not observe any signs of a distinct disk structure or strong spiral arm features within the galaxy's morphology. Faint disturbances are potentially visible near the perimeter, suggestive of recent or ongoing minor interactions or mergers. Overall, the galaxy appears to be a relatively massive system with a relatively low rate of star formation.
