The galaxy presents as an elliptical morphology, with a high degree of central concentration. The core exhibits a bright, relatively uniform, and unresolved appearance. Surrounding this central region is a diffuse halo, with a gradual decrease in luminosity as radial distance increases. There is no visible spiral arm structure, nor is there evidence of a prominent dust lane. The light distribution is smooth and centrally concentrated, consistent with an early-type galaxy. The overall color appears slightly redder toward the center, suggestive of an older stellar population dominating the core. No signs of a recent or ongoing major merger event are evident. The isophotes appear relatively smooth and regular, indicating a relaxed dynamical state. There is a minor hint of a disturbance, but it is very slight.
