The galaxy presents as a lenticular or edge-on spiral type, exhibiting a relatively smooth light distribution across its main body. The central bulge appears bright and concentrated, with a yellowish-white hue, indicating an older stellar population. Extending outwards is a flattened disk component which is tinged with a bluish color on the opposite side of the brighter region, suggestive of ongoing or recent star formation within spiral arms or disk structures. A distinct, reddish region is observed on one end of the galaxy, indicating potential regions of dust obscuration or HII regions associated with localized star formation. The galaxy appears elongated, with a cigar shape profile and some disturbances, possibly due to minor interactions. It does not exhibit a clear spiral structure due to its edge-on orientation.
