The galaxy presents as a largely smooth, elliptical structure with a pronounced central bulge. The light distribution appears centrally concentrated, with a gradual decrease in luminosity moving outward from the core. The galaxy is elongated, and its overall shape is somewhere in between round and cigar-shaped. There's no clear evidence of spiral arm structure or strong dust lanes. Some minor disturbances may be present, but the galaxy doesn't show strong signs of ongoing major merger activity. The color index suggests a population dominated by older stars. The galaxy's relatively compact size is evident.
