The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates into a more diffuse halo. The primary color of the central region is a yellow-red, indicating a potentially older stellar population with lower ongoing star formation. The outer regions of the galaxy appear fainter with a slight blue tint, suggesting the presence of some younger, hotter stars, although it is not highly pronounced. No distinct spiral arms or prominent dust lanes are visible. The overall appearance is consistent with a galaxy that is generally well-settled, with a likely high mass. There might be very slight disturbances in the overall shape, although these are minimal.
