The galaxy presents as a generally smooth, elliptical-like structure. Its morphology is dominated by a central bulge, exhibiting a high degree of luminosity. The overall shape is somewhat elongated, though predominantly round. There is very little evidence of spiral arms or significant disk features; the light distribution appears relatively uniform and concentrated towards the core. Color gradients are subtle, shifting from a bluer hue in the immediate vicinity of the central bulge to a slightly redder tone further out, indicative of potential differences in stellar population or dust content. There is a slight asymmetry to the galactic halo. Interactions with neighboring objects are not readily apparent.
