The galaxy presents as a somewhat elongated structure, approximately cigar-shaped when viewed on the plane of the sky. The light distribution appears relatively smooth, with a dominant central bulge. Faint traces of a disk-like component may be present but lack distinct spiral arm features or concentrated star-forming regions. Color gradients suggest a redder core region transitioning to slightly bluer edges. There is no obvious indication of on-going major merger events or significant tidal disturbances. Minor disturbances may be present, though subtle. Overall the galaxy appears to be a relatively passive system, with a low star formation rate and a considerable amount of stellar mass. 
