The galaxy appears to be a spiral galaxy with a prominent bar structure. The spiral arms are well-defined and loosely wound, tracing a grand design morphology. Two spiral arms are most apparent, but the image resolution does not allow for a precise count. There is evidence of ongoing star formation within the disk, indicated by the blueish hue and some clumpy structure along the arms. The central bulge is moderately sized relative to the disk. The galaxy exhibits an elliptical shape, with the apparent shorter axis of the galaxy appearing approximately one third of the apparent longer axis. There is some evidence for a minor merger or interaction with a smaller dwarf galaxy. The luminosity profile appears to be well-fit by a Sersic profile with an index around 6. There's no indication of an active galactic nucleus. The overall color index suggests a relatively high star formation rate.
