The galaxy presents as an elliptical structure with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Moving outwards, the color transitions to a fainter bluish tinge, suggesting the presence of younger stars and possibly some ongoing star formation within the galaxy's disk. The morphology appears relatively undisturbed with some evidence of a possible disk. The galaxy exhibits an elongated shape, and there's a subtle indication of faint tidal features.
