The galaxy presents as an elliptical morphology, generally smooth in appearance, with little indication of spiral arms or a prominent disk structure. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness away from the core. It exhibits a yellowish-red hue, suggesting a stellar population dominated by older, redder stars and a relative lack of ongoing star formation. The galaxy appears fairly isolated and undisturbed morphologically, with no obvious signs of recent or ongoing major mergers. There is a nearby object that is similar in color to the central galaxy; it could be a smaller satellite galaxy.