The observed galaxy exhibits a centrally concentrated morphology with a relatively smooth, diffuse profile. The overall shape appears somewhere in between round and elliptical, although the isophotes are somewhat irregular. There is some indication of asymmetry or minor disturbances in the outer regions. The galaxy's color gradient appears to be relatively uniform across the visible spectrum, possibly indicating an older stellar population, although this is just a guess based on what I can see. There's a hint of structure that could point toward a past merger event, and it appears the system is not completely relaxed. Further investigation would be needed to fully understand the evolutionary state.
