The galaxy presents a generally smooth appearance with a slightly elongated, cigar-shaped morphology. It exhibits a concentrated central bulge that appears quite luminous, suggesting a significant population of older stars. There is a subtle color gradient visible, with the central region appearing more yellow/orange, potentially indicating an older stellar population and less active star formation in that area, while the outer regions have a slight bluish tint implying the presence of younger, hotter stars. The edges of the galaxy appear somewhat diffuse. There is little evidence of strong spiral arm structure or major dust lanes, supporting the classification of a likely early-type galaxy undergoing some star formation. A small disturbance may be visible in the outer halo of the galaxy.
