The galaxy presents as a relatively smooth, centrally concentrated object, approximately elliptical in shape. The core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There is a subtle color gradient moving outward from the core, with the outer regions appearing slightly redder. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology suggests a possible early-type galaxy with a relatively quiescent star formation history. There may be minor gravitational disturbances, but no major ongoing merger events are visible. The galaxy appears relatively isolated.
