The galaxy presents as a largely featureless elliptical, with a high degree of central concentration. It possesses a slightly elongated, disk-like structure, though lacking the prominent spiral arms typical of grand design galaxies. The color profile indicates older stellar populations dominating, contributing to a relatively smooth and uniform appearance with a discernible red shift. Minimal morphological disturbance is evident, suggesting no recent major merger events. The overall structure appears stable. Evidence of ongoing star formation is low but is still occurring.
