The galaxy appears to be a relatively small, faint spiral galaxy with a disturbed morphology. The spiral arms are somewhat disrupted, showing signs of interaction or recent merger activity. There's a hint of a disk-like structure, but it isn't well-defined or uniform. Blueish regions suggest ongoing star formation, while overall the galaxy exhibits a lower star formation rate. There appears to be an elongated tidal tail extending away from the main body, which may also indicate a galaxy merger. The colors suggest a lower mass system with older stellar populations present throughout. There's also an indication of dust lanes or obscuring material.
