The galaxy presents as an elongated, cigar-shaped structure. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population, possibly an older population. Moving outwards from the core, the luminosity gradually decreases, fading into a more diffuse halo or outer region. The galaxy appears relatively smooth in texture, lacking prominent spiral arms or distinct morphological features. There may be some minor disturbances, but the overall structure is relatively undisturbed. The galaxy has a redshift value that places it at a significant cosmological distance. It displays a distinct red color, indicating the presence of older stellar populations, and possibly a considerable amount of dust obscuring the central regions. The physical size of the galaxy is estimated to be significant, several kiloparsecs in diameter, indicating it is a substantial system.
