The galaxy appears as a relatively compact, elliptical-like object. It is characterized by a smooth, centrally concentrated light profile. The core exhibits a yellowish-orange hue, suggesting a population of older stars. There is a subtle color gradient with the central region appearing more luminous and redder compared to the outer regions which look more diffuse. There is no clear evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a system that has undergone little to no recent major merger events or significant starburst activity. Minor disturbances cannot be ruled out. The rounded appearance indicates a minimal cigar shape to the galaxy.
