This galaxy presents as an edge-on spiral, exhibiting a prominent and relatively bright central bulge. The bulge appears smooth and rounded. A flattened disk is visible, oriented almost perfectly edge-on from our perspective. Dust lanes are suspected, causing some obscuration and color variations within the disk. The disk is more prominent on one side of the bulge than the other.

The galaxy possesses an estimated stellar mass on the higher end. Star formation rate appears to be slow, suggesting that the galaxy is more mature. There's no obvious evidence of a recent major merger, with the overall structure appearing relatively undisturbed.
