The galaxy appears to be a spiral galaxy viewed at an oblique angle. The central bulge is prominent and has a yellowish hue, possibly indicating an older stellar population. Faint spiral arms extend outwards from the central region. It seems to be dominated by two spiral arms, possibly indicating a grand design spiral. The spiral arms are somewhat tightly wound. There is evidence of ongoing star formation within the arms, with the presence of bluer regions scattered throughout, though no HII regions are distinct. The galaxy exhibits a moderate-sized bulge relative to its disk, appearing smaller than the disk. There appears to be a bar running through the center. There is a hint of a tidal disturbance that may be the result of a possible interaction with a smaller dwarf galaxy located at the lower edge of the image. The general morphology suggests it is not undergoing a major merger.