The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The central region exhibits a yellowish-white hue, suggestive of an older stellar population with fewer young, massive stars. There is subtle asymmetry observed in the surrounding halo, which could indicate minor disturbances. There appears to be an area of redder light to the left of the galaxy, as well as an area of bluer light above it. The overall structure appears relatively undisturbed with no obvious spiral arms, bars, or tidal tails. The light from the galaxy appears to be relatively red-shifted overall.
