The galaxy presents as a compact, disk-like structure, exhibiting a bright, concentrated central region. The galaxy's light appears more intense toward the center. Its morphology indicates a possible presence of a central bulge. There is no clear spiral arm structure is apparent, but some minor disturbances may be present. The galaxy shows slight elongation, leaning towards a cigar shape. The blue-ish tint might be indicating active star formation. There is no indication of a major ongoing merger.