The observed galaxy presents a distinct, relatively compact structure. A bright, concentrated central region dominates the galaxy's overall appearance, suggesting the presence of a prominent galactic nucleus. Surrounding this nucleus is a fainter, more diffuse disk-like component. The disk appears relatively smooth and lacks apparent spiral arm structure, hinting at a possible lenticular or early-type spiral morphology. There may be some faint outer ring. Overall, the galaxy exhibits a predominantly blue hue, suggestive of active star formation occurring within the galaxy. No major disturbances in the galaxy's structure are visible.
