The galaxy presents as a relatively compact and concentrated object. It appears largely smooth in texture with no readily apparent spiral arms or prominent dust lanes. The core exhibits a high degree of luminosity that gradually decreases towards the outer regions of the galaxy. The overall shape is approximately elliptical, with a minor deviation from perfect circularity. There are no visible signs of ongoing major mergers or significant tidal disturbances, but there may be a minor disruption to its shape. The colour profile is somewhat redder suggesting a stellar population dominated by older stars, though there is some blue light in the central core.
