The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting characteristics of both elliptical and spiral morphologies. It presents a relatively smooth, centralized bulge with a subtle disk-like component. There is some evidence of faint spiral arm structures. The overall color appears slightly redder, which could indicate an older stellar population and a reduced rate of recent star formation. The galaxy demonstrates an intermediate degree of roundness, not perfectly spherical, but also not highly elongated, more so in between shapes. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is an indication of a minor gravitational disturbance, however it does not seem to have gone under a full merging event.
