This galaxy exhibits a notable elliptical morphology, with an approximate effective radius of 6.8 kpc. The light distribution is relatively smooth, displaying a high degree of central concentration. The galaxy presents a gradual color gradient, transitioning from a yellowish core to a bluer periphery. There is no indication of prominent spiral arms or a distinct disk structure. Based on the observed characteristics, this galaxy is likely an early-type galaxy with an estimated stellar mass greater than 10^10 solar masses. Its star formation rate is relatively low. There is no current evidence of a major merger, but a minor disturbance cannot be ruled out. The axial ratio indicates a shape somewhere between round and elongated.
