The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in surface brightness outwards. The overall shape is moderately rounded. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although some subtle asymmetries hint at possible minor gravitational interactions. The color profile indicates a higher concentration of older stellar populations, with redder hues dominating the central regions and a gradual shift towards slightly bluer tones in the outer regions. The size suggests a relatively massive galaxy. The low presence of features indicates a low rate of star formation.
