The galaxy presents a smooth, rounded morphology, exhibiting minimal discernible features such as spiral arms or a prominent disk structure. The light distribution appears centrally concentrated with a gradual decrease in intensity outwards. Color gradients suggest a redder core transitioning to slightly bluer outer regions. The overall structure indicates a system likely dominated by an older stellar population. There is no visual evidence of ongoing major mergers or significant tidal disturbances, but the possibility of minor interactions cannot be ruled out. The galaxy's compactness is evident, indicating a relatively high stellar density within its core.
