The galaxy appears to be a relatively smooth, elliptical system. The light is concentrated towards the center, forming a bright, yellowish core. The outer regions show a gradual decrease in luminosity and a shift in color toward the redder end of the spectrum, indicating an older stellar population at the edges. There is no prominent disk structure, spiral arms, or irregular features visible, which suggests a dynamically relaxed system. The overall shape is elongated, but not extremely so, appearing more 'in between' round and cigar shaped. There are no obvious signs of an ongoing major merger or tidal disturbances. The color gradients suggest a galaxy where star formation has slowed or ceased in the outer regions, likely leaving behind a population of older, redder stars.
