The galaxy appears to be a spiral type, although the spiral arms are somewhat diffuse. There is a central bulge that appears neither particularly large nor small, but is moderately prominent. The galaxy is not perfectly face-on, as it appears slightly inclined to our line of sight. There is some evidence of a bar-like structure traversing the central bulge. The disk shows indications of active star formation, particularly in the spiral arms where regions of blue light are visible. The galaxy exhibits some disturbed features that may be indicative of a possible minor interaction or past merger event. Overall, it seems to be a well-defined spiral galaxy at a moderate distance.
