The galaxy presents as a somewhat elliptical structure, demonstrating a notable degree of smoothness in its overall morphology. The central region exhibits a concentrated luminosity, indicative of a prominent galactic bulge. The light profile transitions gradually from the core to the outer regions, with a subtle flattening apparent along its major axis. The color gradient suggests a population of older stars within the central bulge, exhibiting a yellowish hue. The outer regions show a bluer tint, which may be due to younger stars or a small amount of star forming regions. Faint extensions hint at minor disturbances or tidal interactions, though the galaxy appears generally undisturbed.
