The galaxy presents as a slightly inclined, disk-shaped system. Its central region exhibits a bright, diffuse glow. The disk appears asymmetric, with a noticeable warping or thickening on one side. Subtle color variations are visible across the disk, with a bluer hue dominating the primary plane and hints of redder regions scattered within. There is an indication of possible disturbances, although its overall structure retains a coherent form, indicating a potentially minor interaction or internal dynamic process. There may be some areas of active star formation visible.
