The galaxy presents as a primarily smooth object with a somewhat elongated, cigar-shaped morphology. A subtle disk-like structure is possibly present, but difficult to discern due to the smoothness and orientation of the galaxy. The central bulge appears to be a yellowish-orange hue, suggesting an older stellar population. The outer regions exhibit a bluer tinge, possibly indicative of ongoing star formation. There are no obvious signs of major mergers or tidal disturbances. The galaxy appears relatively undisturbed. Some minor irregularities may be present, but these are difficult to definitively classify without higher resolution imaging.
