The galaxy presents as a largely smooth, elliptical form. It displays a bright, concentrated central bulge, likely indicative of an older stellar population. The overall color gradient shifts from yellowish-white in the core to a slightly redder hue in the outer regions, suggesting some degree of radial population variation with older stars in the center. There are hints of faint, diffuse structures extending from the central region, though these are not well-defined. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated with no obvious signs of ongoing major merger activity, though subtle disturbances might be present. The overall morphology points toward an early-type galaxy with a significant spheroidal component.
