The galaxy presents a yellowish-white hue, indicating an older stellar population. Its overall form appears to be generally smooth and elliptical but not perfectly round. There may be some evidence of a minor disturbance or a possible interaction with a smaller companion object, given a slight asymmetry in the light distribution. The galaxy exhibits a compact core region, with the light intensity decreasing gradually from the center outward. There is a slight hint of a fainter, more diffuse component surrounding the core. No spiral arms are visible. The features suggest a relatively evolved system, possibly undergoing or having undergone a merger event in the past.
