The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The light distribution suggests a higher density of older stars in the core, with a gradual decrease in stellar density towards the outer regions. There is a slight elongation in shape, deviating from a perfectly circular form, but is far from cigar-shaped. There is no significant evidence of strong spiral arms or complex dust lanes. No clear merging events or major disturbances are visible in the image. The overall color appears slightly redder, consistent with a population of older stars and a relatively low star formation rate.
