The galaxy exhibits a generally elliptical morphology, with a smooth and concentrated central bulge. The bulge appears to be composed of older stellar populations, indicated by its yellowish hue. A faint, disk-like structure surrounds the bulge, displaying a bluer color gradient, suggestive of ongoing or recent star formation. The overall roundness is moderate, leaning more toward an in-between shape than a perfectly circular or elongated form. There are no obvious signs of major tidal disturbances or ongoing merging events, though subtle asymmetries cannot be ruled out at this resolution. The galaxy's light profile appears relatively undisturbed, supporting the assessment of a generally relaxed system.
