The galaxy presents as an elliptical or lenticular morphology, with a relatively smooth light distribution concentrated towards the center. There is a distinct, bright core region, surrounded by a more diffuse halo. Coloration suggests an older stellar population. The overall structure appears undisturbed, but there may be faint tidal features or minor disturbances. A possible merging event could be inferred by a bulge. There is minimal evidence of ongoing star formation. 
