The galaxy presents as a somewhat elliptical, relatively smooth structure with a concentrated central bulge. The primary color is a yellowish-white, suggesting a population of older stars, though there may be some regions exhibiting bluer hues, potentially indicating more recent star formation. There are no prominent spiral arms or bar structures visible. The light distribution appears centrally concentrated. Subtle hints of asymmetry or minor disturbances in the outer regions may suggest possible past interactions or ongoing accretion events, although no definitive merging is apparent.
