The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge which appears bright and slightly yellow in color, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, with hints of bluer regions, particularly at the lower edges of the galaxy, which may indicate ongoing star formation. The overall structure appears relatively undisturbed, showing no obvious signs of tidal interactions or significant morphological irregularities. The galaxy exhibits a weak gradient in color from the center outwards, indicating that the stellar populations and star formation rates vary across its structure.
