The galaxy presents a smooth, elliptical morphology. It appears elongated with a cigar-shaped profile. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is a noticeable color gradient from the center outwards, with the central region exhibiting a more yellowish hue, transitioning to a bluer color in the outer regions. This suggests older stellar populations dominate the core, while younger stars may be forming further out. No signs of strong spiral arm structures or major disturbances are evident, and the galaxy is likely not undergoing a major merging event. There are only minor features present that could indicate minor gravitational disturbances. The overall smooth appearance implies a relatively evolved system.
