This galaxy presents as an elliptical type, exhibiting a smooth, centrally concentrated morphology. The light distribution indicates a lack of prominent spiral arms or distinct features. The object appears elongated, suggesting a significant ellipticity, possibly close to a cigar shape. Its color profile suggests a dominant population of older stars. Based on its morphology, it's likely a quiescent galaxy with a relatively low star formation rate. There is no apparent evidence of any major mergers or tidal disturbances. The light distribution from the galaxy is smooth and appears to have a lack of dust lanes or patches. The object's red-shifted light indicates that is at a significant cosmological distance.
