The galaxy presents as a flattened disk with a prominent central bulge. The galaxy is viewed at an angle, revealing a substantial disk component. Spiral arms are clearly visible extending outwards from the central bulge. The winding of these arms appears to be of medium tightness. Based on the appearance of the spiral arms there are likely two dominant arms. There is no clear evidence of strong tidal disturbances. The galaxy appears relatively isolated, with no indication of ongoing or recent major mergers. The central bulge appears to be of moderate size relative to the overall galaxy. Based on the color distribution, there is evidence of star formation occurring within the disk, most notably along the spiral arms.
