The galaxy presents a largely smooth, elliptical morphology with a moderately concentrated central bulge. Its color profile indicates a population of primarily older stars, suggesting a relatively low rate of current star formation. While largely featureless, there is a slight elongation visible, deviating subtly from a perfectly circular shape. There is no discernible evidence of any ongoing major mergers or significant tidal disturbances in this image. The overall impression is of a galaxy that is relatively evolved and quiescent.
