The galaxy presents a largely smooth, rounded morphology with a concentration of light towards the central region. It is observed at a redshift of approximately 0.154, indicating its considerable distance. The estimated size of the galaxy is roughly 5.14 kiloparsecs in radius.

The galaxy's light is primarily composed of blue and green wavelengths, with a lower percentage of light in redder wavelengths. Given the concentration of light towards the center and the smoothness of the galaxy, this appears to be a relatively mature galaxy. It appears that the galaxy is potentially undergoing a merger, or that the galaxy had a merger event in the past. Overall, the galaxy has characteristics that are consistent with a relatively evolved state. 
