This galaxy appears to be a relatively smooth, elliptical galaxy with a bright central bulge. The galaxy exhibits a generally round shape. Its color profile suggests a population of older stars, with the central region displaying a yellowish hue. There is little evidence of spiral arm structure or significant dust lanes. Minor disturbances might be present but are not readily apparent in the image. The galaxy has an estimated effective radius of approximately 5 kpc, indicating a moderately sized galaxy. Its color is composed of an amalgamation of red, green, and blue light which can be used to infer its approximate age. The redshift indicates that the galaxy is at a considerable cosmological distance. Overall, it resembles a typical early-type galaxy with a dominant spheroid component.