The galaxy presents as a generally smooth, centrally concentrated object with a spheroidal morphology. It exhibits a noticeable color gradient, appearing more yellow-red at the core and gradually transitioning to a bluer hue in the outer regions. There is no visible spiral arm structure or dust lane obscuration apparent in the image. The galaxy's relatively high degree of central concentration suggests it might be an elliptical galaxy, potentially of type E0-E3. There appears to be a smaller, somewhat diffuse companion object nearby, which is likely another galaxy in the same cluster, or potentially interacting with the central object. The overall color suggests an evolved stellar population, though some ongoing star formation may contribute to the bluer outer regions. The galaxy is quite round in appearance. There are no signs of any recent or ongoing mergers.
