The galaxy presents as a primarily smooth structure, centrally concentrated with a slight elongation. A discernible feature is a possible interaction or merging event with a smaller companion galaxy. This secondary component appears as a less luminous concentration of light, offset from the main galactic body. The primary body exhibits a color gradient, with a brighter, bluer core surrounded by a slightly fainter, redder halo. The isophotes of the galaxy exhibit some twisting, potentially indicative of tidal forces or distortions caused by the interaction. Overall, the galaxy appears relatively undisturbed apart from the likely ongoing merging event, as evidenced by the smoothness of the primary body.
