The galaxy presents as a relatively compact structure, exhibiting a mostly smooth morphology. The primary body of the galaxy appears elongated, with a possible slight disturbance or tidal feature visible on one side, suggesting a minor interaction or past merger event. The light distribution is not perfectly symmetrical. The color gradient indicates the presence of older stellar populations, particularly in the central region where a yellowish-orange hue dominates, possibly indicating an elliptical galaxy, but one with minor disturbances in its structure. There may be a smaller object nearby which is a possible merger remnant.
