The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a bright, prominent core. There is a lack of distinct spiral arm structures or dust lanes visible in the image. The galaxy exhibits a moderate ellipticity, appearing somewhat between round and elongated. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a redder hue toward the galactic center. There is no evidence of ongoing major merging activity, though a minor disturbance cannot be ruled out, and low level star formation may be present. The galaxy is estimated to have a substantial mass.
