The galaxy presents as a spiral galaxy with a prominent disk structure. There is evidence of spiral arm structure but they are not clearly defined. The arms appear somewhat flocculent. The galaxy possesses a central bulge, estimated to be of large size. The galaxy is oriented approximately face-on with respect to our line of sight. There is no indication of a strong bar feature. The light distribution within the galaxy appears relatively smooth, suggesting a lack of significant ongoing major star formation. There also appears to be a second, much smaller, spheroidal galaxy close to the larger spiral galaxy. There are no obvious signs of a major merger event, however there is a subtle disturbance on the disk.
