The galaxy presents as a luminous, centrally concentrated object, displaying a generally smooth morphology. The overall shape is elliptical, appearing somewhat elongated but not highly so. A bright, yellowish core is evident, suggesting a concentration of older stars. The outer regions fade gradually, showing a subtle color gradient from yellow-white near the center to a slightly bluer hue in the extended halo. No distinct spiral arms or strong dust lanes are visible. There may be some indications of minor disturbances to the morphology but no definitive evidence of a major merger. The galaxy is likely of significant mass and moderate star formation.
