The galaxy presents as a roughly elliptical form, appearing somewhat elongated. Its core region exhibits a bright, concentrated luminosity, suggesting a significant density of stars or an active galactic nucleus. Moving outward from the core, the light diminishes gradually, with some indication of subtle, diffuse structures. There are no clearly defined spiral arms or a distinct disk component visible in the image. Faint irregularities in the outer regions hint at possible tidal interactions or recent mergers, although no major disturbances are clearly evident. The overall color profile suggests a population of older stars, particularly in the central bulge, with bluer hues concentrated around the outer edges, possibly indicating some recent star formation activity. However, the dominant impression is that of a relatively smooth and evolved system.
