The galaxy presents as a disk galaxy, viewed nearly edge-on. The bulge is quite prominent and appears predominantly round. There is little to no indication of a boxy bulge. A large fraction of the galaxy's light appears to originate from the disk component. There are no strong visual indications of current or recent major merger activity, but there might be minor tidal disturbances. This galaxy appears to be on the larger end of the galaxy spectrum. Based on the galaxy color, star formation rates are thought to be very low.
