The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. The galaxy appears somewhat rounded, with a shape that is neither perfectly spherical nor highly elongated. There is a subtle hint of a disk-like structure, though it is not clearly defined. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the galaxy's morphology, but there is minor disturbance, which may suggest minor interactions. The color indices suggest a relatively evolved stellar population, with a possible ongoing low level star formation.
