The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge. The radial light profile appears consistent with a de Vaucouleurs profile, suggesting an older stellar population. The semi-major axis is approximately twice the length of the semi-minor axis. The isophotes exhibit a slight ellipticity, with the major axis oriented roughly northwest-southeast. There is no resolved spiral structure or apparent star formation regions evident in this color image. The overall color is redder than average, indicative of lower star formation activity. The galaxy exhibits signs of an elliptical shape in the r-band.
