The galaxy presents as a lenticular or early spiral type with a generally smooth morphology. The central bulge is pronounced, displaying a yellowish-orange hue, potentially indicating an older stellar population. A flattened disk component is visible, although the structure is not well-defined with distinct spiral arms. The disk exhibits a greenish tint, possibly suggestive of ongoing star formation. The galaxy appears elongated, with a cigar shape, and the overall structure is undisturbed, with no obvious signs of tidal interactions or major mergers. There may be minor disturbances visible. 
