The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The light distribution suggests a somewhat spheroidal shape, deviating from a perfect circle. There is a slight elongation, possibly indicating a minor interaction or internal dynamics. The galaxy core appears bright, potentially signifying an active galactic nucleus or a high density of stars in that region. The overall color is consistent with an older stellar population. The surface brightness decreases gradually from the center outwards. There are some disturbances in the galaxy shape, indicating a merging event. The redshift indicates that the galaxy is at a significant cosmological distance.
