The galaxy exhibits a disturbed morphology, possibly indicative of a recent or ongoing merger event. The central region shows a complex structure with what appears to be a ring-like feature. The ring is not uniform in color, with distinct regions displaying blue and red hues, suggesting differential star formation or dust obscuration. The overall color of the galaxy is relatively blue, implying the presence of a younger stellar population. There is evidence of tidal tails or disrupted arms, which further supports the hypothesis of a gravitational interaction with another galaxy. The galaxy has a somewhat compact appearance. 
