The galaxy presents a diffuse morphology, appearing largely smooth with some features present. Its shape appears to be somewhat irregular. The light distribution suggests an elliptical-like structure. A significant portion of the observed light is concentrated in what seems to be two brighter regions, or cores, within the galaxy, potentially indicating a pre-merger or post-merger state of interacting galaxies or active galactic nuclei. A considerable amount of disturbance is evident. The general color profile is yellowish, hinting at an older stellar population, although some bluer regions may suggest some ongoing star formation or areas of dust obscuration.
