The galaxy presents a generally smooth, elliptical morphology. A central bulge is visible, appearing bright and concentrated. The galaxy exhibits a color gradient, with the core region showing a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge is a more diffuse halo of light. A slight hint of bluer colors can be detected in the outer regions of the galaxy, potentially suggestive of ongoing, though subdued, star formation. There is no clear indication of spiral arms or a defined disk structure. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers with other galaxies. There may be some very subtle asymmetrical features, suggesting minor past gravitational disturbances. The roundness suggests the galaxy is likely an E0-E2 galaxy. 
