The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer regions. There is a yellow-red hue to the central region, indicative of an older stellar population. The outer edges are less defined, with a hint of a halo. There is no discernible spiral arm structure. The galaxy shows some signs of minor disturbances but does not appear to be undergoing a major merger. The galaxy exhibits a high degree of overall symmetry, with an approximate redshift of 0.168537 and it is relatively massive. Based on the overall color and morphology, the galaxy is likely to have a low star formation rate.
