The galaxy presents as a spiral type, viewed at an oblique angle relative to our line of sight, but not quite edge-on. There is a distinct central bulge with a high degree of luminosity, and a defined bar structure appears to traverse this bulge along its major axis. Two prominent spiral arms emanate from the ends of the bar structure, exhibiting a relatively tightly wound morphology. The disk component shows a patchy distribution of light, indicating the presence of both young, star-forming regions and older stellar populations. There may be some indication of minor gravitational disturbance or interaction with another object. The galaxy does not appear to have a dominant bulge. Overall, the galaxy displays a well-defined structure, indicative of a mature spiral galaxy.
