The galaxy presents as a moderately luminous, disk-shaped structure. Its central region exhibits a concentrated, bright bulge that graduates smoothly outwards. The light in this central region appears slightly redder in color. The disk itself displays a somewhat asymmetrical morphology. Fainter, bluish light extends beyond the central bulge, indicating the presence of younger stellar populations and potential ongoing star formation. The outer regions of the galaxy show signs of disturbances or tidal interactions, exhibiting irregularities in its overall form. The galaxy's shape can be characterized as in-between round and cigar shaped, with some visible disturbances that suggest a recent or ongoing merger. 
