The galaxy appears to be a spiral galaxy viewed edge-on, exhibiting a distinct disk-like morphology. A prominent central bulge is visible, displaying a concentrated and bright luminosity. The disk component shows a decrease in luminosity extending outwards. Dust lanes or other obscuring material are suggested by some unevenness in color and light distribution, but the resolution is too low to definitively identify them. The galaxy appears elongated with an axis ratio of approximately 0.5, oriented at roughly 135 degrees counter-clockwise from the horizontal axis. The light from the galaxy is brightest in redder wavelengths with the presence of light in the green and blue wavelengths as well. The overall color index suggests an intermediate population of stars within the galaxy. There are no obvious signs of interaction or significant morphological disturbances.
