The galaxy presents a somewhat amorphous morphology with a dominant bluish hue, suggestive of active star formation. The light is primarily concentrated in what appears to be an elongated central region, but lacks well-defined spiral arms or a distinct nucleus. There is evidence of some disruption or tidal features extending from the main body, indicating that the galaxy might be undergoing an interaction or merger. The overall structure suggests a system that is not fully relaxed, possibly a recent merger or a galaxy undergoing significant internal disturbances. The size is relatively small, hinting at a low mass system.

