The galaxy presents as a relatively smooth, disk-shaped structure with an apparent elliptical morphology. There is a notable central bulge region that appears brighter and more concentrated. The disk component exhibits a flattened profile with what appears to be a tightly wound spiral structure, though it appears largely featureless. Color gradients are subtle, with the central bulge exhibiting a slightly redder hue compared to the surrounding disk, which appears more blue-green. The galaxy appears to be relatively isolated, showing no obvious signs of ongoing major mergers or tidal disturbances, though minor disturbances cannot be ruled out. Overall, the galaxy presents a quiescent appearance with little to no signs of active star formation in the disk, although this may be due to resolution limitations.
