The galaxy appears to be a relatively smooth, centrally concentrated system. The morphology suggests a dominant spheroidal component. The light distribution is fairly symmetrical, with a gradual decrease in intensity from the core outward. There is little evidence of spiral arms or a distinct disk. The galaxy exhibits a slightly elliptical shape but is largely round in appearance. Any disturbances from possible minor mergers appear faint, and there is little evidence of active star formation. The galaxy shows a population of older stars with a redder color. It seems like a quiescent, evolved galaxy.
