The galaxy appears to be a relatively smooth, elliptical or lenticular system, with a noticeable bulge. The light is concentrated towards the center. The galaxy appears elongated, with a cigar shape. The overall color profile suggests a population of older stars, contributing to a yellowish hue, though hints of bluer light near the edges hint at some star formation. There is no strong indication of ongoing major mergers, though there could be a minor interaction causing some disturbance in the system. The galaxy appears to be of substantial mass.
