The galaxy appears to be a relatively smooth, elliptical system, with a concentrated central bulge. There is a noticeable radial gradient in color and luminosity, transitioning from a bluer central region to a redder, more diffuse outer halo. The object presents a slightly elongated morphology, deviating subtly from a perfect circle. There is no apparent presence of strong spiral arm structures or other significant features suggesting an actively merging state, though minor tidal disturbances may be present. The color suggests the presence of both younger, bluer stars in the core and an older, redder stellar population dominating the outer regions. The overall structure is generally undisturbed, indicating a stable and relatively quiescent system.
