The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears more yellow in color, indicative of an older stellar population. Fainter, somewhat diffuse green and reddish hues are present at the galaxy's periphery, possibly indicating more recent, yet subdued star formation within cooler gas and dust. The overall round shape of the galaxy suggests that it is likely an early-type galaxy, lacking prominent spiral arms or a well-defined disk. There is no obvious evidence of ongoing major mergers or tidal disturbances. 
