The galaxy presents a morphology indicative of an elliptical or lenticular type. Its light distribution is generally smooth and concentrated towards the center. There is a slight elongation, but no discernible spiral arm structure or prominent dust lanes are visible. The core appears as a bright, unresolved nucleus. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a slightly bluer outer region, possibly indicating some ongoing, low-level star formation activity. The overall appearance suggests a galaxy that is relatively evolved, with a large fraction of its stellar population being older stars. There is a possible merger or tidal disturbance, which is supported by the irregular morphology in the outer region and the presence of a nearby companion galaxy. 
