The galaxy presents as a single, somewhat amorphous structure. There is an uneven distribution of light across the galaxy's body, with the presence of one relatively bright, slightly elongated region, along with another compact area of significantly higher luminosity. These luminous areas are connected by a less dense, but still apparent galactic body. Coloration suggests a mixed stellar population, exhibiting both bluer regions which may indicate ongoing or recent star formation and redder areas which might be attributed to older stellar populations or dust obscuration. The overall shape does not strongly suggest a spiral or elliptical morphology but may be indicative of a galaxy undergoing or having recently undergone a merger or interaction, resulting in the observed irregular form. A possible tidal feature extending away from the main body is not distinct, but hinted at. The galaxy has a moderately high redshift, indicating a considerable distance.
