The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing nearly round from our vantage point. There is no clear evidence of a distinct disk component or spiral arm structure. The light profile suggests a gradual decline in brightness from the center outwards, with the central region appearing as a bright, somewhat diffuse core. Faint color variations are visible throughout the galaxy, with bluer hues interspersed with redder regions in the galaxy indicating regions of active star formation. There is no obvious strong tidal disturbance or signature of a major merger event; it appears to be relatively isolated and undisturbed.
