The galaxy exhibits a flattened, elongated morphology, suggesting an elliptical or lenticular type. The central region appears brighter and more concentrated, with a yellowish hue, possibly indicative of an older stellar population. Fainter, bluer regions extend from the central bulge, hinting at ongoing or recent star formation within a disk-like component. The galaxy is significantly tilted with respect to our line of sight, providing a view of its overall structure. There is a slight asymmetry to the outer regions. The surface brightness appears smooth, with no prominent dust lanes or spiral arm structures clearly visible in the image.
