The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution. The galaxy core appears bright, with the luminosity decreasing gradually towards the outer regions. The shape is elongated, approximated as cigar-shaped. There is a noticeable lack of distinct spiral arms or prominent dust lanes. No features indicative of a major merger event are obviously present. The overall color is on the redder side, indicative of an older stellar population and reduced recent star formation. Based on the red-shift measurement, this galaxy is at a considerable cosmological distance.
