The galaxy presents as a relatively smooth and elliptical-like structure. It exhibits a concentrated central bulge that appears brighter than the surrounding regions. The galaxy's light profile seems to fade gradually outwards from the center, lacking any distinct spiral arm features or prominent dust lanes that would otherwise suggest significant star formation. The color distribution is such that the core appears to have a yellowish-white tint, becoming slightly redder towards the outer edges. The overall appearance is indicative of a galaxy with an older stellar population, possibly a lenticular or early-type spiral galaxy transitioning to a more quiescent state, with suppressed star formation. There appears to be evidence of minor disturbances in the morphology. The galaxy seems to be in a state of interaction, potentially merging with a much smaller, less luminous dwarf galaxy.
