The galaxy presents a generally smooth, elliptical morphology. It appears moderately flattened, exhibiting a shape somewhere between round and elongated. The central region displays a concentration of light, suggesting a prominent galactic nucleus or bulge. The color profile shifts from a more yellowish hue at the core to a slightly bluer tint in the outer regions. The light distribution suggests a population of older stars concentrated in the central bulge, with a possible younger stellar population contributing to the bluer color in the outskirts. There is no visible evidence of strong disturbances, major mergers, or prominent spiral arm structures. Faint irregularities or distortions can be observed, potentially hinting at minor gravitational interactions or past merger events, but these are not distinct.
