This galaxy presents a somewhat elliptical morphology. It displays a prominent central bulge region that exhibits a bright, concentrated luminosity, suggestive of a high density of stars and possibly a supermassive black hole at its core.

Extending outwards from the central bulge, we observe a flattened disk structure. The disk appears relatively smooth. There is no discernible spiral arm structure within the visible portion of the disk. The color distribution across the galaxy suggests a gradient, with the central bulge exhibiting a slightly redder hue compared to the disk, indicating potentially older stellar populations in the bulge and younger stars in the disk. Faint tidal features, potentially resulting from a minor disturbance or past interaction, are possibly present.
