The galaxy presents an elliptical morphology, appearing largely smooth and centralized in the image. There is a concentrated central bulge exhibiting a yellow-orange hue, which suggests a population of older stars. The overall light distribution is relatively uniform, with a gradual decrease in intensity moving outward from the center. There is little to no evidence of spiral arms or distinct substructure within the galaxy; there does not appear to be any dust. A slight elongation is visible, but no tidal tails are seen.
