The galaxy presents a largely smooth, elliptical morphology. It is a relatively round system, exhibiting a high degree of central concentration. The galaxy's core region shows a bright, almost stellar-like appearance. Moving outward from the core, the luminosity gradually decreases into an extended halo. There is little to no evidence of spiral arm structure or prominent dust lanes. No significant morphological disturbances are visible, suggesting the absence of recent major merger events. The overall color is reddish, indicative of an older stellar population and lower ongoing star formation.
