The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated core. The light distribution suggests a dominant spheroidal component. There is little evidence of distinct spiral arms or significant dust lanes, though the outskirts of the object appear slightly more diffuse. The galaxy displays a yellowish-orange hue overall, implying a population of older stars. There is a hint of a possible tidal interaction or minor merger event, as evidenced by a slight distortion and/or an interacting companion galaxy located near the primary object. The isophotes of the galaxy appear to be moderately elliptical but trending toward round.
