The galaxy presents a generally smooth morphology, with a somewhat elliptical appearance. A notable central bulge exhibits a yellowish-orange hue, potentially indicating an older stellar population. Extending outwards from the bulge is a fainter, more diffuse disk with a bluish tint. The overall structure suggests it could be an early-type spiral galaxy or perhaps an elliptical galaxy with some residual star formation. There is evidence of a minor disturbance within the galaxy, as it does not appear entirely uniform. This could be due to a recent minor merger event or internal dynamic processes.
