This galaxy exhibits a generally smooth morphology, with a centrally concentrated luminosity profile. The core region appears roughly circular.

There is evidence of some extended faint structure beyond the central concentration, potentially indicative of a weak disk or tidal features. The color profile suggests a population of older stars, particularly in the central bulge region, which exhibits a more yellow-orange hue. The bluer colors observed in the outer regions indicate some ongoing star formation, though likely at a relatively low rate. The overall appearance suggests a relatively evolved galaxy, possibly in a transitional stage between a spiral and an elliptical morphology, but leaning more towards the elliptical. There is a hint of minor disturbance visible.