The galaxy presents as a relatively compact, disk-like structure with a centrally concentrated bulge. The overall color suggests a mix of stellar populations, with a brighter, somewhat bluer core. This likely indicates ongoing or recent star formation in the central regions. The outer regions of the disk appear fainter and redder. The disk inclination is clearly not face-on, showing an elliptical shape with some warping. This galaxy is likely not undergoing a major merger, but has potentially experienced minor disturbances.
