The galaxy presents a clear spiral structure, viewed at a slight angle relative to face-on. Spiral arms are evident, though somewhat flocculent in nature, extending outwards from a bright central bulge. The bulge itself appears to be of moderate size. The color gradient suggests a well developed galactic structure. The spiral arms exhibit a mottled appearance, which may imply the presence of active star-forming regions within the disk. There is no clear indication of a strong central bar, but the possibility of a weak bar presence cannot be ruled out due to the resolution and the viewing angle. The galaxy does not appear to be undergoing any major merging events. There might be a minor asymmetry or disturbance present in the outer disk, however. The overall morphology points towards a relatively mature spiral galaxy with ongoing, but perhaps not exceptionally high, star formation activity.
