The galaxy presents as an elliptical morphology with a high degree of central concentration. Its overall shape is roughly rounded, with a slight elongation. The light distribution appears smooth with no discernible spiral arms or prominent features. The galaxy exhibits a color gradient, with a redder core transitioning to slightly bluer hues in the outer regions. The red core indicates a high concentration of older stars. The blue outer regions suggest the presence of some younger stellar populations, though to a lesser extent. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances.
