The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of circularity. There is a noticeable radial color gradient, shifting from a bluer hue at the outer edges to a yellow-white core, suggestive of an older stellar population dominating the central region. No distinct spiral arm structures or significant dust lanes are discernible. There are some very faint features towards the outer regions of the galaxy that are indicative of either a disk or that the galaxy may have experienced minor disturbance events. There is no indication of any tidal tails or mergers happening with the galaxy.
