The galaxy presents a distinct spiral structure. The arms are relatively well-defined and exhibit a loosely wound morphology, suggesting it may be a late-type spiral. These arms are populated with regions of active star formation, indicated by their blueish color. These regions are not particularly large or widespread, but they are easily seen.

The galaxy possesses a noticeable bulge at its center. The bulge does not appear to be particularly dominant compared to the disk but has a moderate presence. The bulge also appears relatively smooth, with no obvious signs of complex structure.

There is no obvious presence of a strong central bar feature. The overall shape of the galaxy suggests it is viewed at a slightly oblique angle, perhaps less than 10 degrees off from edge-on. The galaxy has a median effective radius that is quite modest.

There may be minor disturbances due to interactions or mergers, but there is no strong, evident disruption of the galaxy’s main structure. It appears to be relatively isolated, without any other major companion galaxies in close proximity.
