The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a roughly spheroidal shape, transitioning gradually in intensity from the core outwards. There is no distinct disk structure visible. The overall color profile indicates a redder, older stellar population, as evidenced by the greater intensity of the red channel compared to blue or green. Some minor irregularities in the outer regions suggest the possibility of minor tidal disturbances or past interactions.
