The galaxy presents as an elongated, cigar-shaped structure, suggesting it is likely an edge-on spiral or a lenticular galaxy viewed at an oblique angle. A prominent bulge, appearing reddish-orange, is located at one end of the galaxy's major axis. This central region is the brightest and most concentrated part of the galaxy.

A faint, bluish hue extends away from the bulge, forming the main body of the galaxy. This color suggests the presence of younger, hotter stars, indicating regions of active star formation. There appears to be a slight warping to the main disk of the galaxy. There are no obvious signs of strong tidal disturbances or interactions with other galaxies.
