The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions smoothly into a surrounding halo. The core appears brighter, suggesting a higher concentration of older stellar populations or potentially the presence of an active galactic nucleus, although no distinct features of an AGN are visually apparent. The overall color of the central region is reddish, possibly indicating the presence of older, cooler stars. The outer regions show some faint, diffuse blue hues, which could indicate the presence of some younger stellar populations, although their contribution is minimal. There are no prominent spiral arms or distinct dust lanes visible, reinforcing the classification as an elliptical-type galaxy. There is no evidence of significant tidal disturbances or ongoing major merger activity. It appears to be a relatively undisturbed, evolved system.
