The galaxy presents as a centrally concentrated object, exhibiting a generally elliptical morphology. Its core region appears bright and somewhat diffuse, indicating a substantial stellar population, possibly older stars. The light gently fades towards the outer regions. There is a suggestion of a disk structure surrounding the bulge, this is subtle. The color index suggests a mix of stellar populations, but it appears slightly redder, suggesting a somewhat aged stellar population. The lack of prominent dust lanes or active star-forming regions implies a relatively quiescent state. There is no evidence of significant tidal interactions or major mergers in this image.
