The galaxy presents as a largely featureless, elliptical structure with a highly concentrated central bulge that diminishes into a smooth halo. The light distribution appears very uniform and symmetrical. The galaxy has a yellowish hue in the central region, which graduates toward redder tones in the outer areas. The absence of distinct spiral arms, dust lanes, or irregular features suggests an evolved stellar population. The galaxy's overall appearance hints towards a relatively low star formation rate. There is a subtle elongation, but the galaxy primarily has a spherical shape. No evidence of major mergers or significant tidal disturbances are observed in this image, however some small disturbances may be present.
