The galaxy presents an elongated morphology, appearing somewhat cigar-shaped. The core region exhibits a yellowish-white hue, indicating a likely concentration of older stellar populations. This central region is surrounded by a greenish halo, possibly suggesting the presence of younger stars and ionized gas. The overall light distribution appears relatively smooth, lacking prominent spiral arm structures or significant dust lanes. There is a faint extension of light emanating from the galaxy, further suggesting a disturbed morphology or tidal interactions, but without clear evidence of a major merger event. The galaxy is not perfectly symmetrical, appearing somewhat perturbed. The redshift suggests that this galaxy is at a considerable cosmological distance. The relatively blue-green color suggests ongoing star formation, however, the overall smooth appearance points toward an elliptical galaxy, or possibly a lenticular galaxy seen edge-on with moderate star formation activity.
