The galaxy presents as a moderately bright, elongated structure, likely an elliptical galaxy or a spiral galaxy viewed edge-on. The central bulge is pronounced, displaying a concentrated luminosity. The light profile suggests a smooth, featureless morphology, without any prominent spiral arms or dust lanes visible. The colour appears to be generally red-shifted, indicating older stellar populations. The overall appearance suggests a galaxy undergoing minimal star formation at present, but may have a substantial stellar mass. There is some evidence of minor disturbances in the outer regions, possibly indicative of past interactions or mergers.
