The galaxy presents as a centrally concentrated, elliptical form with a generally smooth appearance. A bright, yellowish core region dominates, suggesting a concentration of older stellar populations. The light profile appears to fade gradually from the center outwards. There is a slight elongation visible in the galaxy's shape, moving it away from a perfectly spherical form towards a more cigar-shaped structure. No distinct spiral arms or features indicative of ongoing major star formation are readily apparent from this view. The galaxy's color suggests a relatively low ongoing star formation rate. There are no clear signs of mergers or major disturbances in the surrounding regions of the galaxy.
