The galaxy presents a slightly elongated morphology, appearing as an intermediate form between a perfect circle and a cigar shape. It seems to be dominated by a smooth light distribution, with only subtle features discernible within its structure. A small disturbance appears visible, potentially due to a minor interaction or internal dynamics, but it is difficult to assess the nature of the disturbance. The light from the galaxy suggests a redshift of 0.053970, placing it at a substantial cosmological distance. The bluer light suggests the galaxy is currently forming stars but at a low rate. The mass of the galaxy is in the range of 10^8 solar masses.
