The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The galaxy appears to be quite round, with a slight elongation or disturbance noted along one axis. Faint, indistinct bluer regions are observed in the outer areas of the galaxy, hinting at pockets of recent or ongoing star formation, though this activity appears subdued overall. There is no strong evidence of spiral arm structure or a prominent disk. No obvious signs of an ongoing major merger event are present, although subtle asymmetries may indicate a past interaction or minor disturbance. The overall morphology appears to be consistent with an early-type galaxy.
