The galaxy presents a generally smooth, elliptical morphology. It appears moderately luminous, with a concentrated central bulge that graduates outward into a fainter, more diffuse halo. The color profile indicates a dominant population of older stars, evidenced by the yellowish-orange hue in the central region, though there is a subtle hint of blue star formation in the outer disk. The overall structure is largely undisturbed, showing no signs of major mergers or tidal interactions. Minor disturbances are present, indicated by faint, asymmetric features extending from the main body of the galaxy, possibly indicative of minor interactions or internal processes. There are no clear indications of spiral arm structure. The overall shape is predominantly round, with a slight elongation.
