The galaxy appears as a moderately luminous, gravitationally bound system. It is characterized by a somewhat amorphous structure, exhibiting neither a dominant spheroidal bulge nor well-defined spiral arms. The overall morphology appears to be in between round and elliptical. The light distribution is relatively smooth, with hints of some irregular features or disturbances, potentially indicative of tidal interactions or past merger events. A significant portion of the galaxy's light appears to be concentrated within a central region, suggesting a moderately high stellar density in that area. The overall color appears slightly more red than blue.
