The galaxy appears to be an elliptical type, exhibiting a smooth, spheroidal morphology. Its color profile suggests a population of older stars, trending towards redder hues. There is little evidence of spiral arms or significant dust lanes. The overall light distribution is centrally concentrated, indicative of a dominant bulge component. No obvious signs of recent or ongoing major mergers are apparent, although there could be minor tidal disturbances present within the light profile. The galaxy shows no prominent features associated with active star formation regions. The galaxy has an apparent rounded shape. Overall, this galaxy presents as a relatively passive elliptical, consistent with a system nearing the end of its evolutionary lifecycle.
