The galaxy presents an elliptical morphology, characterized by a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish hue, suggesting a population of older stars. There is a gradual decrease in luminosity moving outwards from the center, with the outer regions appearing more diffuse and tinged with redder hues, possibly indicating a lower density of stars or the presence of dust. The overall structure appears relatively undisturbed, without any prominent tidal features or signs of active merging. There is a minimal presence of blue light, which indicates there isn't a very high population of young stars. The galaxy exhibits moderate roundness.
