The galaxy presents as an elongated, elliptical structure. The central region exhibits a relatively smooth, concentrated light distribution, suggesting a prominent bulge. The overall color of the galaxy appears to be yellowish-white, indicative of an older stellar population with fewer young, blue stars. There is little evidence of spiral arms or active star formation regions. The light falls off gradually from the core to the outer edges. The galaxy appears relatively undisturbed, without any major signs of tidal distortions or ongoing mergers, although a very slight asymmetry cannot be ruled out.
