The galaxy presents as a centrally concentrated, elliptical morphology. Its light profile is smooth and relatively featureless, lacking defined spiral arms or a prominent disk structure. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light gradually diminishes towards the outer edges, appearing more reddish. The object is reasonably round in shape, with only a slight deviation from perfect circularity. There is no evidence of tidal tails, galactic mergers, or other significant disturbances. It is likely a well-established galaxy with a relatively low rate of star formation.
