The galaxy appears as a compact object with an estimated Petrosian half-light radius suggesting a small physical extent. Overall color is bluish-green, indicating the presence of younger, hotter stars and regions of active star formation. There is no obvious spiral structure or well-defined features. Hints of tidal disruptions are visible in the form of faint streamers extending outward from the main body of the galaxy. This would indicate the galaxy has undergone a minor merger. The absence of a prominent bulge, and the overall morphology, suggest it could be an irregular galaxy. It might have formed after a major interaction.
