The galaxy presents as a relatively compact object, displaying a generally smooth morphology. There is minimal evidence of spiral arm structure or significant dust lanes. The light distribution appears centrally concentrated, hinting at an elliptical or lenticular classification. The overall color profile suggests a population dominated by older stars, with a lack of intense blue regions indicative of active star formation. There is a slight elongation to the shape of the galaxy. No obvious signs of major merger activity are apparent, although there is subtle evidence suggesting possible tidal interactions or minor disturbances within the galactic halo.
