The galaxy presents a largely featureless appearance, exhibiting a smooth and rounded morphology. The light distribution appears centrally concentrated, diminishing gradually towards the outer edges. Its color profile suggests a dominant population of older stars, as indicated by the reddish-yellow hue. There are no prominent spiral arms or distinct dust lanes visible. Evidence of tidal disturbances or ongoing major mergers is lacking; although the galaxy's shape suggests that minor merging cannot be ruled out. The object is observed to be relatively compact in size, though possessing a substantial mass. Observed redshift indicates considerable distance, which is consistent with the absolute magnitudes.
