The galaxy presents as a flattened, elliptical structure with a smooth, diffuse light distribution. A prominent central bulge exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, the disk appears elongated and displays a bluer tint, potentially indicating the presence of younger, hotter stars or ongoing star formation. Faint, extended features hint at a possible disk structure, though these are not clearly defined. The overall appearance suggests a galaxy undergoing a transition from a more spheroidal to a disk-dominated morphology or vice versa, showing evidence of past or ongoing interactions that may have influenced its shape and star formation activity. There are slight disturbances observed within the galactic disc, suggesting minor interactions may have occurred. The observed redshift suggests a considerable distance, affecting the detailed observation of finer structures within the galaxy.
