The galaxy presents as a somewhat elliptical, moderately compact system. It exhibits a smooth light distribution, lacking any prominent spiral arms or bar structure. The core region displays a concentrated yellowish-white hue, possibly indicating a population of older stars. Fainter, bluer, irregular features extend from the central region, potentially indicating regions of ongoing or recent star formation. There are no signs of major mergers or significant tidal disturbances, with only minor asymmetries present. Overall, the galaxy appears relatively undisturbed.
