The galaxy presents as a relatively compact, elliptical system, with a smooth, featureless appearance indicative of an older stellar population. Its morphology suggests a well-mixed structure. The galaxy exhibits a generally round shape. The dominant color appears to be a pale yellowish-white hue in the center and edges, implying a stellar population dominated by older, evolved stars. No prominent spiral arms or dust lanes are visible. There are no distinct signs of any major ongoing merger activity or significant tidal disturbances, but there may be minor indications of a disturbance.
