The galaxy presents as an elongated, ellipsoidal structure with a distinct central bulge. The light distribution suggests a concentration of older stellar populations, likely composed primarily of Population II stars, dominating the central region, inferred from the yellow-orange hue. The outer regions appear fainter and exhibit a bluer tint, which could indicate the presence of younger stars and some ongoing, albeit relatively low, star formation. There is no indication of a prominent spiral arm structure or a central bar. The overall morphology suggests a galaxy that is tending towards an elliptical form. There are no signs of major tidal disturbances or ongoing mergers, though subtle asymmetries or minor disturbances cannot be ruled out at this resolution. The galaxy's smooth appearance suggests a dynamically evolved system.
