The galaxy presents a generally smooth morphology, appearing largely featureless in this observation. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core gradually fading into a less luminous, more diffuse outer region. The overall shape is elliptical, approaching circular, with no strong evidence of spiral arm structures or bar features. There is a very subtle suggestion of a disk-like structure, but it is not sharply defined. Color gradients are observed, with the central region appearing more yellow/red, potentially indicating an older stellar population, while the outer regions have a bluer tint, which may indicate younger stars. There are no obvious signs of ongoing major merging activity or significant tidal disturbances.
