The object presents as a spiral galaxy, though the structure is notably disturbed. Two bright, concentrated regions are apparent near the galaxy's core, possibly indicative of an ongoing or recent merger event or the presence of a strong bar structure. Broad, loosely wound spiral arms emanate from the central region, displaying a patchy distribution of star formation. The color gradient suggests active star formation in these arms, exhibiting a bluer hue, while the central region appears redder, indicating an older stellar population or increased dust obscuration. Overall, the galaxy exhibits signs of significant dynamical activity and a relatively high rate of star formation, possibly induced by the merger or interaction process. The galaxy does not appear to be edge-on. There is no obvious dust lane.
