The galaxy appears to be a relatively small elliptical galaxy at a significant distance. Its light is redshifted. The galaxy exhibits a smooth, centrally concentrated luminosity profile. The shape of the galaxy is generally elliptical, appearing more "in-between" round and cigar shaped. There is no obvious presence of spiral arms or a prominent disk component. The galaxy's central region is characterized by a yellow-orange hue, likely indicating an older stellar population with fewer hot, young stars and a prevalence of redder stars. A slight hint of bluer light is seen on the outskirts, potentially indicative of ongoing, but low levels of, star formation. There is no obvious major disturbance to the galaxy's overall structure, such as tidal tails or significant asymmetries, that would suggest a recent major merger event, though minor disturbances are possible.
