The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent dust lane obscures the central bulge, which appears slightly more yellow than the outer disk. The disk exhibits a smooth, elongated structure, with a suggestion of warping or tidal disturbance at the lower end. The lack of distinct spiral arm features indicates a relatively quiescent star formation rate, consistent with its classification. Overall, it appears to be a relatively massive galaxy, but not exceptionally so.
