The galaxy presents as a largely featureless, elliptical morphology. The light profile indicates a centrally concentrated spheroid. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. The outer regions appear fainter, gradually fading into the background sky, showing a more reddish color. There is a slight asymmetry in the outer isophotes, possibly indicative of a minor disturbance or past interaction. No distinct spiral arms or dust lanes are discernible. The overall smooth appearance and color distribution suggest a relatively evolved galaxy with a low current star formation rate.
