The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly round, showing a slight elongation. Its core is notably bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. Proceeding outward from the nucleus, the luminosity diminishes smoothly, blending into a more diffuse halo region with a slight reddish tint. There are no prominent spiral arms or distinct dust lanes visible. The overall light distribution suggests a system dominated by evolved stars, with a low ongoing star formation rate. There is no signs of tidal features or distortions to indicate recent major merger activity, but there is a possible minor disturbance. The galaxy displays an intermediate axis ratio, falling somewhere between a perfect circle and a very elongated ellipsoid.
