The galaxy presents a largely smooth, elliptical morphology with a noticeable central bulge that graduates into a surrounding halo. There is some indication of a disk-like structure, though not distinctly defined. The galaxy appears to be a relatively undisturbed system, showing no obvious signs of ongoing mergers or major tidal disturbances.

The central bulge is characterized by a yellowish hue, suggesting an older stellar population. The surrounding region exhibits a bluer color, indicative of ongoing star formation. The overall structure appears rather rounded, with no clear elongation. While there might be some minor asymmetry, it does not seem to significantly impact the overall shape.
