The galaxy presents a largely smooth, elliptical morphology. There is little evidence of spiral arms or significant disk structure. Its color is a relatively uniform yellowish-white, suggestive of an older stellar population with fewer young, hot, blue stars. The galaxy appears moderately concentrated, with a gradual decrease in luminosity from the core outwards. There is a slight deviation from perfect roundness, appearing more like an ellipse than a perfect circle. There is no strong evidence of an ongoing major merger, although a slight asymmetry might indicate a minor interaction or disturbance. No prominent dust lanes or regions of intense star formation are immediately apparent within the galaxy's structure.
