The galaxy presents as a system of two distinct components. One component appears as a relatively smooth and rounded structure, while the other exhibits a more elongated, disk-like morphology. The rounded component displays a more concentrated central region, with a luminosity gradient that decreases smoothly outwards. The disk-like component is characterized by a flatter appearance and shows some hints of internal structure, though at this resolution, features are not sharply defined. The color of the rounded component appears slightly bluer compared to the disk-like component, which shows more yellow and red colors. There may be some subtle interaction or tidal features connecting the two components, but they are not strongly evident. A significant fraction of the light is concentrated within a radius of approximately 4 kpc.
