This galaxy presents as a somewhat elongated structure, likely a disk galaxy seen at a high inclination. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. The disk appears relatively smooth, with a subtle bluish tint suggesting regions of ongoing star formation, most prominent along the edges of the galaxy. The shape of the disk is relatively undisturbed, showing only a minor distortion or asymmetry. There is no obvious sign of a major merger.
