This galaxy exhibits a generally smooth morphology with a pronounced, elongated shape. Its central region displays a bright, concentrated luminosity, suggestive of a substantial stellar population or potentially an active galactic nucleus. Moving outward from the center, the luminosity gradually diminishes, forming a diffuse halo. There's a subtle color gradient across the galaxy, transitioning from a warmer, possibly older stellar population in the core, to slightly cooler hues in the outer regions, indicating potentially younger stars or ongoing star formation. There's no obvious presence of spiral arms or significant dust lanes.
