The galaxy presents a largely smooth, elliptical morphology. The light is concentrated towards the center, exhibiting a bright, yellowish core, indicating a significant population of older stars. There is a slight extension of fainter, bluer light surrounding the central region, possibly indicating the presence of a faint, diffuse disk or halo component with ongoing, albeit low-level, star formation. The overall structure appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. There is a subtle colour gradient from the core outwards.
