This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light distribution suggests a somewhat spheroidal shape, with a high degree of symmetry. There's a gradual decrease in luminosity from the core outwards, giving the galaxy a diffuse appearance at its outer edges. The overall color is indicative of an older stellar population. There is potentially a minor companion galaxy or background object that appears close to the main galaxy. There is no clear evidence of spiral arms, dust lanes, or recent major merger activity.
