This galaxy presents as a relatively smooth and centrally concentrated object. The light profile appears diffuse, with a bright core that gradually fades outward into the surrounding halo. The overall shape is somewhere in-between round and elliptical, with a slight elongation. There is no indication of any spiral arm structure or prominent dust lanes. The light distribution suggests an absence of significant ongoing major mergers or tidal disturbances, with only minor disturbances possibly present. The galaxy displays a color gradient, appearing bluer in the central region, suggestive of recent or ongoing star formation, and becoming redder towards the outer regions, indicating an older stellar population.
