The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. A pronounced central bulge is visible, exhibiting a brighter, more concentrated luminosity compared to the rest of the disk. The bulge appears slightly elongated along the major axis of the galaxy. The disk itself shows a gradient in brightness, with intensity decreasing from the central bulge outwards. Some evidence of dust lanes or spiral arm fragments are visible in a portion of the disk. The overall color suggests a mixed stellar population, with bluer hues near the central region and yellower/redder tones extending outwards in the disk. There may be some evidence of a weak interaction occurring in this galaxy.
