The galaxy presents as a fairly compact object with a moderate redshift, indicating it is at a considerable distance. It appears elliptical in shape, with a significant axis ratio suggesting it is highly elongated. The color profile indicates a concentration of older stellar populations, particularly in the central region, which exhibits a yellowish hue. There is minimal evidence of spiral arm structure or significant dust lanes. The outer regions show a subtle falloff in luminosity. Based on its morphology, the galaxy likely has a smooth light distribution, typical of an early-type system. Possible minor disturbances are present within the galaxy.