The galaxy exhibits a generally smooth morphology. The dominant feature is a bright, centrally concentrated bulge that appears nearly spherical. There are no visible spiral arms or strong indications of a disk structure, though some faint, diffuse extensions of light may indicate the presence of a very faint, disturbed disk component. The color profile is indicative of a substantial population of older stars, with the central bulge presenting a reddish-yellow hue. There is some evidence of ongoing star formation, particularly in the outer regions, as suggested by the faint blue-green tinge in the outer halo. There is no evidence of any major mergers or significant tidal disturbances in this image, though minor distortions may be present.
