The galaxy presents as a fairly smooth and elliptical structure. It exhibits a concentrated, bright central bulge that dominates the light profile. The color gradient suggests a population of older stars. The overall morphology appears undisturbed, with no prominent signs of tidal features, major asymmetries, or ongoing merger activity. There may be some hint of a faint disk structure. Overall, this galaxy appears to be a relatively undisturbed system with ongoing star formation at a specific rate which might be considered normal for such a galaxy.
