The galaxy presents a primarily smooth morphology, with an elliptical appearance. Its shape is moderately elongated. The central region exhibits a higher luminosity, transitioning to a less luminous halo. The color gradient indicates a population of older stars concentrated in the central bulge, suggested by the redder hue. There's a hint of a disk structure and some blue coloration towards the outer regions, indicating the presence of younger stars. There is no apparent interaction or major disturbance of the galaxy's structure. The overall structure appears consistent with a galaxy in a relatively quiescent state.
