The galaxy presents a largely smooth and rounded morphology. The overall light distribution is centrally concentrated with a noticeable decrease in intensity towards the outer regions. It exhibits a subtle color gradient, transitioning from a more yellow-white hue in the core to a slightly bluer color in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears to be relatively isolated, showing no prominent signs of tidal interaction or ongoing mergers, although a minor disturbance cannot be ruled out. Overall, the galaxy appears to be an early-type galaxy, possibly an elliptical or lenticular galaxy.
