The galaxy presents as an elliptical form, appearing largely smooth in texture. A color gradient is observable with a concentration of yellow towards the center, indicating a high density of older stellar populations in the bulge. The outer regions display a blueish tint, which may imply younger stars and ongoing, albeit subdued, star formation. The overall structure suggests a dynamically relaxed system. There appears to be no significant spiral arm structure or dust lane obscuration, further reinforcing its classification as an elliptical galaxy. The aspect ratio suggests a slightly elongated shape, but not to the point of a highly flattened disk system. There is a faint hint of some minor disturbances in the outer halo, but the galaxy appears to be relatively isolated and undisturbed.
