The object appears to be a disk galaxy, viewed at an oblique angle, but relatively close to edge-on. A central bulge is visible, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk component is primarily bluish, indicating the presence of younger, hotter stars and active star formation. There is a notable asymmetry in the disk structure. One side extends further than the other and has lower surface brightness. There also seems to be significant dust and gas obscuration on the right side of the disk. Irregularities in the disk and the extended feature suggest possible tidal interactions or a recent merger event. The galaxy has a smooth appearance, but with some features present.
