The galaxy presents a generally smooth, elliptical morphology. A bright central bulge dominates the overall structure, exhibiting a concentrated luminosity profile that fades outwards towards the edges. The shape is somewhere between round and elongated. There may be a hint of a faint, diffuse disk component. There is no obvious evidence of strong spiral arm structure or any kind of major merging activity. However, there may be a very slight disturbance in the galactic halo of the galaxy, with a small distortion on its periphery that could be due to a minor interaction with a smaller object, but further analysis is needed. Color gradients suggest a moderate presence of younger stellar populations. The color appears bluer in the less concentrated parts of the galaxy and redder in its core.
