This galaxy appears to be a spiral galaxy, observed at a slight angle from edge-on, though features suggest it is not a pure edge-on disk. Spiral arms are discernible, though not sharply defined, suggesting a flocculent spiral structure. The arms exhibit a bluish hue, indicative of ongoing star formation activity.

The central bulge is present, and its size is not exceptionally prominent, appearing moderately sized. The color of the bulge is generally consistent with an older stellar population. There is no obvious bar structure.

Overall, the galaxy displays some signs of disturbance or interaction, as the spiral arms are not entirely smooth and symmetric. There is a degree of irregularity.

Given its relatively small size and morphology, this galaxy has a moderate amount of stellar mass and a low star formation rate.
