The galaxy presents an edge-on disk morphology. There is a prominent central bulge, the shape of which appears somewhat rounded. The disk component is smooth with very little observed structure or resolved star forming regions. There is very faint evidence of a dust lane bisecting the galaxy. Overall, the galaxy exhibits a bluish color, suggesting that its stellar population is primarily composed of relatively young stars, though there is some light emitted across the visible spectrum from a redder population as well. There is no evidence of any current merger activity or tidal disturbances, which would otherwise significantly alter the disk structure.
