The galaxy presents as a spiral type, viewed edge-on from our vantage point. A prominent, moderately-sized central bulge is observed. The bulge appears yellowish-white, suggesting an older stellar population. The disk of the galaxy appears thin and elongated, exhibiting a bluish hue, indicative of ongoing star formation. The arms are not clearly resolved due to the edge-on orientation. No significant signs of major mergers or tidal disturbances are readily apparent. There is potentially some weak bar structure in the galaxy.
