The galaxy presents as a relatively smooth, elliptical-like structure with an apparent high degree of central concentration. The light distribution suggests it is primarily spheroidal in shape, though there is some indication of possible tidal features or minor disturbances. The color index shows a dominance of redder wavelengths, which might indicate an older stellar population, a higher metallicity, and suppressed star formation. There are areas with enhanced redness to one side of the galaxy, which could be due to dust reddening the observed light. Overall, this galaxy looks to be in the later stages of its evolution.
