The galaxy presents with a somewhat amorphous morphology. Its central region appears moderately concentrated but lacks a distinct bulge. A faint disk-like structure may be present, but is significantly disturbed. Several regions of intense blue emission are distributed throughout the galaxy. These indicate active star formation regions, concentrated in what appears to be a tidal feature. The galaxy appears to be involved in a minor merger or tidal interaction, as evidenced by the disturbed morphology and apparent tidal tail extending from the main body. Overall, the galaxy presents with characteristics suggesting a complex and potentially ongoing interaction or merging event, resulting in active star formation in its outer regions.
