The galaxy presents a disk-like structure, viewed at an angle that is not perfectly edge-on but close to face-on. Prominent spiral arm features are clearly visible, extending outward from a central bulge. The spiral arms appear somewhat fragmented and asymmetrical, suggesting possible interactions or disturbances within the galaxy. The central bulge is substantial and appears to be quite luminous, indicating a large concentration of stars, potentially an older stellar population. A bar feature seems to bisect the galaxy through the center of the bulge and extending past it.

Overall, the galaxy exhibits characteristics of a spiral galaxy with a relatively high rate of star formation, showing a mix of stellar populations and signs of dynamical activity.
