The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a population of older stars, leaning towards redder hues, with minimal evidence of active star formation. There's a subtle gradient in color and intensity, with the core being the brightest and reddest part of the galaxy. The galaxy exhibits a high degree of roundness in its overall shape, appearing almost spherical, with only very slight deviations from perfect circularity. There is no discernible evidence of ongoing or recent major mergers or tidal disturbances in the system.
