The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The overall shape appears elliptical, transitioning from a brighter, roughly circular core region to a more elongated outer halo. There is a slight asymmetry in the outer isophotes, possibly indicating a minor interaction or tidal disturbance. Color gradients are present, with the central region appearing more yellow-orange and the outer regions exhibiting a bluer hue. This suggests a population of older stars in the core and a younger stellar population or ongoing star formation in the outskirts. The galaxy appears to be relatively isolated, showing no strong evidence of major merger activity based on significant distortions or tidal tails, although minor disturbances cannot be ruled out.
