The galaxy presents as a spiral type. Distinct spiral arms are visible, though somewhat flocculent in nature, displaying a patchy distribution of star-forming regions. The galaxy's central bulge is subtle, with a moderate contribution to the overall luminosity profile. There is a suggestion of a bar structure across the central region of the galaxy. The disk appears slightly disturbed or warped, showing asymmetry which might indicate gravitational interaction with another galaxy. There are some signs of possible tidal debris in the form of faint, diffuse extensions which is also indicative of merger activity.
