The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright core that appears yellowish-white in color, indicative of an older stellar population. Progressing outwards from the core, the galaxy displays a gradual decrease in brightness. Faint, diffuse extensions are observed on opposing sides of the central core, possibly suggesting a flattened disk or an elongated spheroidal shape. The lack of distinct spiral arms or prominent dust lanes suggests a relatively quiescent state in terms of star formation, with a greater population of older stars dominating its light output. There's no evidence of strong tidal features or distortions, indicating a lack of recent major merger events. The overall morphology leans towards a disk galaxy or perhaps a lenticular galaxy given its smooth structure. The galaxy is redshifted, indicating a significant distance, therefore the galaxy is being observed at a younger stage in its life cycle.
