The galaxy presents a morphology indicative of a relatively smooth structure, with a degree of roundness to its overall shape. There is an impression of a central, concentrated bulge region which exhibits a slightly warmer color profile than its surrounding extended halo. This suggests older stellar populations in the core. The outer regions show a more diffuse, cooler color, possibly indicative of more recent star formation or a younger stellar population. There is no strong evidence of spiral arm structures or a highly disturbed morphology, indicating a relatively settled state for the system. There may be a hint of minor disturbance in the galaxy's outer halo but this is not certain. Based on the available evidence, the galaxy appears to be a relatively massive system with ongoing star formation.
