The galaxy presents as a relatively smooth, elliptical or lenticular object. It appears elongated, but not dramatically so, suggesting an axial ratio that is somewhat close to unity. There is a central concentration of light, which appears to be brightest in the central region of the galaxy, suggesting the presence of a bulge. Color gradients across the galaxy are subtle, with a slightly bluer tint in the outer regions compared to the core. This could be indicative of ongoing, but low levels of, star formation in the galactic disk. The galaxy lacks any obvious spiral arm structures or strong dust lanes, reinforcing the classification as either elliptical or lenticular. The overall morphology suggests a system that is relatively evolved.
