The galaxy presents as a centrally concentrated, fairly smooth object with a slight elongation. There is a bright core region with a more diffuse halo surrounding it. The color appears somewhat blueish white, though with hints of yellower regions. There might be some minor disturbances indicating a possible interaction or merger. Overall, the galaxy appears to be relatively massive and exhibiting ongoing, potentially significant, star formation activity. The light distribution suggests it may be an early-type spiral galaxy, with a prominent bulge.
