The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile is centrally peaked, suggesting a prominent bulge component. The overall shape appears to be moderately elliptical, tending towards round. There is a hint of disk-like structure, but it is not sharply defined.

The color gradient appears to show a slightly redder core, indicative of an older stellar population. The outer regions show bluer colors which suggest the existence of younger star populations within the galaxy.

There are hints of minor disturbance, possibly indicating the presence of tidal features or ongoing minor mergers, but no clear sign of a major ongoing merger event. Overall, the galaxy appears to be a relatively undisturbed system.
