The galaxy presents as a resolved object with a generally elliptical morphology, although some subtle features suggest the possible presence of a disk component. The central region exhibits a higher surface brightness and appears yellowish, indicative of an older stellar population. Moving outward, the color shifts towards a bluer hue, suggesting the presence of younger stars and ongoing or recent star formation in the outer regions. There is a hint of spiral structure within the disk, although it is not well-defined. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a small irregularity within the disk, indicating minor gravitational disturbances. The galaxy displays a smooth appearance and high roundness.
