The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color gradient suggests an older stellar population, appearing more yellow-red in the central region, indicative of lower star formation activity. The overall structure appears largely undisturbed, without prominent tidal features or signs of major mergers. The absence of distinct spiral arms or significant dust lanes reinforces its classification as an elliptical or lenticular galaxy with a substantial stellar mass. The galaxy appears to be relatively isolated with no major companions visible in close proximity.
