The galaxy appears to be an elliptical type, characterized by a smooth, diffuse light distribution. It exhibits an overall golden hue, suggesting an older stellar population. There is minimal evidence of spiral arms or significant dust lanes. The galaxy's shape is mostly rounded but is somewhat elongated, presenting a moderate degree of ellipticity. Faint hints of tidal disturbances suggest a potential past interaction or minor merger event. The object's low star formation rate is consistent with the evolved appearance.
