The galaxy presents an elliptical morphology. It appears largely smooth in structure, with a high degree of central concentration that gradually fades towards its periphery. The isophotes suggest a slightly elongated shape, transitioning between round and cigar shaped. There is no discernable spiral arm structure or significant dust lane obscuration evident in this image. There are no signs of any major merger events, though subtle disturbances might be present. Its redshift indicates the galaxy is at a moderate cosmological distance.
