This galaxy appears to be a spiral galaxy, observed at a high inclination. The central bulge is bright and concentrated. A faint disk is observable. There is some evidence of asymmetry or minor tidal disruption in the outer disk, possibly indicative of a past or ongoing minor merger event. The galaxy has a relatively smooth appearance, but does show possible faint spiral arm structures. The galaxy exhibits blue colors in its outer regions and a reddish central bulge, suggesting ongoing star formation in the disk and an older stellar population in the bulge. There is no obvious central bar. 
