The galaxy presents a roughly circular morphology, appearing relatively compact. It exhibits a bright, concentrated central region, potentially indicative of an active galactic nucleus or a dense stellar population. The core demonstrates a blue-white hue, suggesting the presence of young, hot stars. Fainter, somewhat disturbed material is asymmetrically distributed around the central region. It shows a redder coloration in some areas surrounding the central region. The asymmetric structures suggest the galaxy might have undergone a minor interaction or disturbance event. The overall smooth appearance suggests the galaxy is not a late stage major merger, although faint tidal features cannot be ruled out.
