The galaxy presents as a spiral disk galaxy, observed nearly edge-on from our vantage point. A prominent central bulge dominates the galaxy's morphology. The bulge exhibits a smooth, concentrated distribution of light, appearing approximately round. The disk appears very thin, characteristic of an edge-on orientation. Faint arms extend from the bulge. The color distribution suggests a relatively old stellar population, and low star formation rate within the bulge, in contrast with the disk which displays bluer colors. There are no obvious signs of major tidal disturbances or ongoing mergers. There is no bar structure visible.
