The galaxy presents as a disk galaxy, viewed at a moderate inclination. Its overall form appears relatively smooth, with a concentration of light towards the center suggesting a bulge. The galaxy exhibits a flattened, somewhat elongated shape. There are no prominent spiral arms visible. A region of possibly active star formation is present at one end of the disk, displaying a slightly reddish hue. No signs of a major merger are evident, though there is a slight hint of a minor disturbance in the overall symmetry. The dominant color of the galaxy is blue-white, indicative of a moderate population of relatively young, hot stars.
