The galaxy presents as a smooth, elongated structure, highly suggestive of an elliptical morphology observed at an oblique angle. The central region exhibits a higher concentration of luminosity, gradually diminishing towards the outer edges. A distinct color gradient is visible, transitioning from a predominantly yellowish-orange core to a fainter, slightly bluer halo. The lack of discernible spiral arms or dust lanes reinforces the classification of this galaxy as an early-type, possibly an elliptical or lenticular galaxy. There is a subtle suggestion of minor tidal disturbance or interaction on the periphery, though no clear merger events are visible. Overall, this galaxy appears to be a relatively mature system, with subdued star formation activity implied by the redder central colors and smooth structure.
