The galaxy presents as a lenticular or early-type spiral system, exhibiting a smooth, centralized bulge with a gradual decrease in luminosity outward. There is little to no presence of defined spiral arm structure, indicating a relatively quiescent morphology. The galaxy exhibits a pale blue hue throughout, likely due to a population of younger stars with ongoing, albeit low, levels of star formation. The galaxy's overall shape is elliptical and leans towards being round with some flattening observed, but it is not highly elongated. No signs of major tidal disturbances or ongoing mergers are apparent, though subtle asymmetries may indicate minor interactions. 
