The galaxy presents as a moderately luminous, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. Moving outwards from the center, the luminosity gradually decreases, forming a smooth, diffuse halo. There are no distinct spiral arms or prominent dust lanes visible, consistent with a relatively featureless morphology. The color appears yellowish, indicating a stellar population that is dominated by older, redder stars. A slight elongation is discernible, suggesting it is not perfectly spherical, but more of a flattened spheroid. There is no strong evidence of recent or ongoing major mergers or tidal interactions. The smooth profile and color indices point towards an evolved system with minimal ongoing star formation. The overall structure is indicative of a relatively massive galaxy.
