The galaxy appears to be a relatively smooth, elliptical system. It exhibits a generally round morphology, lacking any prominent disk-like structures or spiral arms. A bright, concentrated core region is evident, suggestive of a substantial central bulge. The galaxy's light profile appears to be relatively uniform, without obvious signs of major tidal distortions or ongoing mergers. The color gradient suggests a population of older stars, particularly within the central regions, as indicated by the redder hues. Some faint, diffuse blue light is discernible in the outer regions, possibly indicating the presence of some younger stars or ongoing, but low-level, star formation. The galaxy lacks obvious signs of significant dust lanes or prominent star-forming regions.
