The galaxy presents as a concentrated, centrally-dominated system. It appears to be elliptical in shape, with a smooth, featureless light profile across the visible spectrum. A bright central bulge is evident, gradually decreasing in intensity outward to the galaxy's edge. The galaxy exhibits a color gradient; its central region is more yellowish, possibly indicating an older stellar population, whereas the outer regions show slightly bluer hues. The disk is seen nearly edge on, with little dust and gas. There is no evidence of spiral arm structure or ongoing star formation. It appears relatively isolated, showing no obvious signs of tidal disturbances or interactions with neighboring galaxies.
