The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo or disk. The light is concentrated towards the center, with a distinct yellow-orange hue, suggesting a population of older stars and a relatively low rate of current star formation. There is no apparent spiral structure, distinct dust lanes, or significant tidal features indicating recent major merger events. The galaxy possesses a generally rounded shape with no significant elongation or asymmetry.
