The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light distribution appears centrally symmetric, exhibiting a near-circular isophotal shape. There is a marked color gradient, with a yellow-white hue dominating the core region, transitioning to a redder color in the outer regions. There is little evidence of spiral arm structure or prominent dust lanes. The overall appearance suggests a spheroid-dominated system. There is no indication of any recent or ongoing major merger events. Minor disturbances may be present.
