The galaxy presents as a relatively smooth and concentrated light distribution. It appears somewhat elliptical in shape, tending toward roundness. The central region exhibits a higher surface brightness, indicative of a bulge component. There is subtle color variation; the core is predominantly yellow-white, with a hint of bluer light distributed in the outer regions. This suggests a mix of older stellar populations in the bulge and some younger, star-forming regions in what might be a faint disk. There is no strong evidence of spiral arm structures or a prominent disk. The overall morphology suggests an early-type spiral galaxy or a late-type elliptical galaxy. There is some marginal evidence of a minor disturbance in the morphology; however, there is no conclusive evidence of ongoing major mergers or interactions.
