The galaxy presents as a relatively compact, disc-shaped structure. A bright central bulge is evident, surrounded by a fainter, more diffuse disk. The disk appears somewhat disturbed, with a non-uniform distribution of light. There are hints of asymmetry in the outer regions, possibly indicating a tidal interaction or recent merger event. There is some degree of blueness in the galaxy, suggesting the presence of recent star formation. The smoothness of the object is questionable based on visual inspection, with the presence of potentially irregular features. Overall, the galaxy appears to be actively evolving, displaying a mixture of smooth and disturbed morphologies.
