The galaxy presents as a spiral structure, although with some distortion apparent in its morphology. There is no clear, large central bulge, and the arms appear somewhat disrupted or flocculent, indicative of possible tidal interactions or mergers in its past or ongoing. A significant fraction of its light appears to be emitted from these arms.

The galaxy exhibits a range of stellar populations as traced by colour variations across its structure. Some regions show bluer tints, suggesting active star formation, while other regions are redder, possibly indicating older stellar populations or higher dust content. These younger stars suggest a relatively high star formation rate.

There appears to be a faint halo or extended emission surrounding the central region, which could be attributed to scattered light, tidal debris, or a diffuse stellar component. The system is estimated to be fairly massive. Overall, this galaxy appears to be dynamically active and has been undergoing significant evolutionary processes.
