The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a concentration towards the galactic center, gradually decreasing towards the outer regions. The primary body of the galaxy appears largely spheroidal. There is a noticeable color gradient, with a yellowish-white hue dominating the central region, potentially indicating an older stellar population. The outer regions exhibit a slightly bluer tint. There is a small visual disturbance or interaction occurring which may suggest a minor merger.
