The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a notable radial color gradient, appearing more yellow-red towards the core and transitioning to a slightly bluer hue in the outer regions. There is no apparent spiral arm structure or evidence of a prominent disk. The galaxy appears relatively undisturbed, with only subtle indications of minor irregularities in its outer isophotes, potentially hinting at past or ongoing minor interactions. The overall structure suggests a system dominated by an older stellar population, with a modest ongoing star formation rate. The lack of strong morphological disturbances indicates it is not currently undergoing a major merger.
