The galaxy presents as an elliptical structure with a smooth, concentrated central bulge. The overall color gradient suggests a population of older stars, trending towards redder hues at the galactic center. The outer regions exhibit a fainter, bluer color, possibly indicating the presence of a younger stellar population, though at a significantly lower star formation rate overall. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a slight deviation from perfect circularity, appearing slightly elongated. There are subtle indications of minor gravitational disturbance, possibly due to an ongoing or past minor merger event. Overall, the galaxy appears to be a massive, relatively quiescent system with a primarily evolved stellar population.
