The galaxy presents as a moderately bright, disk-shaped structure viewed at a slight angle. The central region exhibits a concentrated, yellowish-white glow suggestive of an older stellar population. The outer regions of the galaxy transition to a greenish hue, indicating the presence of ongoing star formation, potentially with a mix of younger, hotter stars and ionized gas. The disk appears relatively smooth, lacking prominent spiral arm structures. The overall morphology is consistent with a galaxy undergoing quiescent star formation with an elliptical-like shape. There may be a faint dust lane present on the top of the galaxy, but the resolution limits a more precise measurement.
