The galaxy presents as an elliptical morphology, appearing generally smooth in structure, with a high degree of central concentration. It exhibits a color profile that indicates a relatively evolved stellar population. There is a slight asymmetry in the distribution of light, suggesting a possible minor disturbance. The absence of prominent spiral arms and a relatively homogenous color distribution further supports its classification as an elliptical galaxy. The reddish hue indicates that it is not particularly active in terms of star formation.
