The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. Its color profile suggests a population dominated by older stars, exhibiting a yellow-red hue with an apparent lack of significant blue star formation. The galaxy appears relatively isolated, though there is a nearby object that may be tidally interacting with it. No prominent dust lanes or spiral arm structures are discernible within the limitations of the image resolution. The shape of the galaxy leans towards being in between round and elliptical. There is no obvious evidence of a major merger event, though some minor disturbance cannot be ruled out completely.