The galaxy presents as a centrally concentrated object with a relatively smooth light distribution. The morphology appears primarily elliptical, lacking any clear spiral arm structure or bar. The core region exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. The light intensity decreases gradually from the center outwards, showing a smooth transition into the fainter outer regions. There are no obvious signs of recent major merger events or strong tidal interactions. The galaxy appears generally undisturbed. The object is moderately compact. The color profile indicates a relatively red color overall, characteristic of a galaxy dominated by an older stellar population with ongoing moderate star formation. The smoothness of the light profile suggests that it is unlikely to be a disk galaxy seen face-on.
