The galaxy presents as a somewhat diffuse, centrally concentrated object. It exhibits a generally smooth morphology, although there is evidence of disturbed features. There may be a merger event in progress. The central region appears relatively circular, while the outer regions show irregularities and asymmetries. The galaxy exhibits a color gradient, transitioning from bluer hues in some regions to redder tones elsewhere, suggesting variations in stellar populations or dust content. The overall color profile suggests a significant population of older stars, but with ongoing or recent star formation activity in certain regions.
