The galaxy appears to be a spiral galaxy viewed edge-on. It exhibits a noticeable bulge at its center, which is a bright, yellowish-white hue, suggesting a population of older stars. The disk component is elongated, with a slight warp. The primary axis of the disk exhibits a blueish tint, indicative of ongoing star formation. The dust lane is not particularly prominent, but can be inferred to be aligned with the primary axis due to the color gradient.

The overall structure is relatively smooth, and the galaxy doesn't show any strong signs of tidal disturbances or ongoing mergers, though there appears to be a small disturbance visible at the farthest extent of one end of the disk, potentially suggesting a past or ongoing minor interaction. The galaxy is classified as having moderate mass and, based on the colors present, has a lower star formation rate.
