The galaxy exhibits a moderately defined disk-like structure. It appears to be undergoing some form of interaction or disturbance as evidenced by asymmetry and some possible tidal features or disrupted spiral arms. Color gradients are visible within the galaxy, suggesting a varying stellar population distribution. The central region is relatively bright, possibly indicating a high concentration of stars and potentially an active galactic nucleus. The overall color profile suggests ongoing star formation, possibly triggered by the interaction. Its estimated size suggests it is a dwarf galaxy.
