The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. There is a concentrated central bulge that appears nearly featureless. Its shape is subtly elongated; between a perfect circle and cigar-shaped, and its light profile smoothly diminishes from the core outward, with no distinct spiral arm structures or prominent dust lanes discernible. Faint, diffuse extensions are noted on either side of the galaxy. There is no evidence of ongoing major merger activity or significant tidal disturbances, though the faint extensions imply that there could have been a minor disturbance at some time. The galaxy's light is primarily redshifted, with the strongest emission in the red portion of the spectrum.
