The galaxy presents as a relatively smooth, centrally concentrated object, with a high degree of symmetry and a noticeable lack of distinct spiral arm structures. The light distribution appears to follow a profile that increases sharply toward the center, indicating a bulge-dominated morphology. There is some evidence of subtle color variations, with a yellowish central region possibly indicative of an older stellar population and regions of faint blue possibly indicating some star formation. The overall shape appears slightly elliptical. There are no obvious signs of mergers or major disturbances in the galaxy's morphology.
