The galaxy presents as a lenticular, elongated structure with a smooth appearance. A prominent central bulge exhibits a yellowish hue, indicative of an older stellar population. Fainter blueish light traces the outer disk, suggesting ongoing, though relatively low, star formation within spiral arm structures that are not clearly defined. The major axis of the galaxy extends significantly compared to its minor axis, giving it a cigar-like shape. There is no immediately obvious sign of tidal interactions or major disturbances in its morphology, suggesting it is in a relatively quiescent state and not undergoing a major merger.
