The galaxy exhibits a relatively smooth morphology with a discernible elliptical shape. The color profile indicates a higher concentration of redder light in the central bulge, suggesting an older stellar population. The outer regions display bluer hues, potentially indicative of more recent star formation activity. The galaxy's overall structure appears relatively undisturbed, with no significant signs of major mergers or tidal disruptions. The elliptical shape is moderately elongated with a minor axis ratio indicating some degree of flattening. The galaxy's light is centrally concentrated, consistent with a Sersic profile.
