The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing more round than elongated. The core region displays a bright, yellowish-white hue, suggesting an older stellar population. Fainter, bluer light surrounds the core, indicating the presence of younger stars. The galaxy shows some potential signs of minor disturbances, but the overall structure doesn't seem heavily disrupted. No clear spiral arm structure is observed. There may be very faint tidal features.
