The galaxy presents as a single, relatively smooth structure with a centrally concentrated light profile. It appears largely featureless, lacking distinct spiral arms or a prominent bar. The core exhibits a yellowish hue, potentially indicating an older stellar population, while the outer regions display a slightly bluer color. The galaxy appears somewhat elongated but not extremely so. There is no clear indication of any major ongoing mergers or significant tidal disturbances, although there is a slight asymmetry in the outer halo, suggesting there may have been minor interaction in the past.
