The galaxy appears to be elliptical in shape, possessing a smooth, relatively featureless morphology. The light distribution suggests a concentrated central bulge, surrounded by a more diffuse halo. There is a noticeable color gradient, with the core exhibiting a yellowish hue, transitioning to a bluer color in the outer regions. This color difference may indicate variations in stellar populations. There is little evidence of spiral arms or significant dust lanes. The galaxy appears isolated, without signs of any major mergers or tidal interactions. The lack of morphological disturbances suggests it is a relatively undisturbed system.
