The galaxy presents as a centrally concentrated object with a largely smooth morphology. The light distribution suggests a roughly elliptical shape, exhibiting a significant degree of roundness, with minimal elongation. The color appears predominantly yellowish, possibly indicating an older stellar population. There is little evidence of spiral arm structure or significant dust lanes from this perspective, suggesting that it may be a lenticular or elliptical galaxy. There are potentially minor disturbances in the outer regions, but overall, the galaxy seems to be relatively undisturbed with no prominent signs of ongoing merger activity. The object subtends a small angular size, consistent with its significant distance.
