The galaxy presents a morphology that is neither purely elliptical nor a well-defined spiral. It appears to be in a state of disturbance, possibly undergoing a merging event with a smaller galaxy, or exhibiting tidal interactions.

The central region has a high concentration of older stars, indicating it is dominated by an older stellar population.

The outer regions show less defined spiral arm structures, with some indication of bluer, younger stars present, which implies ongoing or recent star formation activity in these regions. Patches of blue light are apparent, which may show the location of nebulae and young star clusters. 

There is evidence of potential tidal features or extended stellar streams, suggesting gravitational interactions. Overall, the galaxy presents a complex morphology indicative of recent or ongoing interactions that are actively influencing its star formation and overall structure.
