The galaxy presents as a relatively small, elongated structure. Its overall shape is somewhat cigar-like, lacking a pronounced central bulge or disk. The light distribution appears smooth, with no obvious spiral arms or distinct features. The color is generally uniform across the galaxy, showing a bias toward redder wavelengths. There is no strong indication of significant recent star formation. Based on its morphology, the galaxy may be undergoing, or have recently undergone, a minor interaction or disturbance. There is no obvious presence of a major merger or any other strong distortion to its overall form.
