The galaxy presents an elliptical morphology with a smooth, relatively uniform light distribution. It exhibits a bright, concentrated central bulge that appears to be composed of older stellar populations, indicated by its yellowish-orange hue. The galaxy gradually fades outwards from the core, without any obvious spiral arm structures or dust lanes visible. There is some slight asymmetry in the outer regions. Given the estimated size and color, the galaxy is consistent with a massive elliptical galaxy at a redshift of approximately 0.336, suggesting a significant distance from our own.
