This galaxy presents as a moderately luminous object, exhibiting a red-shifted spectrum indicative of a significant cosmological distance. The morphological characteristics suggest a relatively smooth, somewhat elliptical appearance. The galaxy's light distribution appears concentrated, with a noticeable central bulge. Faint hints of a surrounding disk-like structure are potentially present but not clearly defined. Irregularities in its morphology suggest potential interactions or mergers. The galaxy exhibits reddish hues, possibly indicating an older stellar population and/or significant dust extinction.
