The galaxy exhibits a smooth, elliptical morphology. The central region is a bright, concentrated yellowish-white, suggesting an older stellar population. There is a gradual falloff in brightness from the core outwards into the less defined, fuzzier, outer regions. A subtle color gradient exists, with the outermost parts appearing slightly bluer, indicating the presence of some younger stars or ongoing star formation, although at a relatively low rate. The galaxy appears to be relatively undisturbed, without any obvious signs of major mergers or tidal interactions. Its overall structure is consistent with a large galaxy that has undergone significant aging of its stellar populations. The galaxy is slightly elongated with an axial ratio of around 0.9, its inclination angle is rather small.
