The galaxy presents as an elongated, edge-on or highly inclined disk galaxy. A distinct central bulge is observed, appearing as a concentrated region of brighter, yellowish-white light. Fainter blue arms appear to extend from the bulge, suggesting a significant population of young, hot stars. A substantial dust lane seems to bisect the galaxy. The lack of clear spiral structure suggests the galaxy's star formation is relatively uniform across its disk, or obscured by dust. Overall, the galaxy exhibits the characteristics of a typical disk galaxy viewed at a high inclination, with evidence of ongoing star formation. There is a slight warp apparent to the galaxy.
