The galaxy presents as a spiral galaxy, viewed at an oblique angle, but close to edge-on. A prominent central bulge is visible, with a concentrated, bright yellow-white hue, suggesting an older stellar population. The disk component exhibits a mottled texture with blue regions indicating areas of active star formation. Faint dust lanes are also visible. The galaxy exhibits signs of spiral arms. A weak bar structure appears to be present in the center of the galaxy. There are no major signs of merging, although there is some slight distortion of the disk indicating possible minor interactions. The estimated size of the galaxy is about 4 kpc in radius.
