The galaxy presents as a system comprised of two distinct components. The larger of the two appears as a disk galaxy with a bright, concentrated central region, possibly indicating an active galactic nucleus or a region of intense star formation. The disk exhibits a mottled appearance, potentially indicative of spiral arm structure, although the image resolution limits detailed analysis. The color is primarily bluish-green, suggesting the presence of young, hot stars.

The second component is smaller and more elongated. Its color is primarily orange-red, possibly indicating an older stellar population. It shows some indications of tidal disturbance, suggesting an interaction with the larger galaxy. A merging event or close gravitational interaction with the larger disk galaxy cannot be ruled out based on the data presented. The estimated size of the larger galaxy is a few kiloparsecs across.
