The galaxy presents as a centrally concentrated system, exhibiting a smooth, largely featureless appearance. The light profile increases sharply toward the center. There is a distinct bulge component that dominates the overall morphology. The color appears largely homogenous across the galaxy, trending slightly redder in the central region, which could indicate an older stellar population. There is little evidence of spiral arm structure or dust lanes. The galaxy's shape is approximately elliptical but appears more elongated than circular. There does not seem to be any current significant interaction or merging activity occurring with the object.
