The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular galaxy given its smooth, featureless morphology. The central bulge exhibits a yellowish-white color, suggesting an older stellar population. The outer regions of the galaxy appear more diffuse and somewhat elongated, exhibiting a slight disk-like structure but lacking defined spiral arms. There is minimal evidence of ongoing star formation. No signs of strong tidal distortions or merging activity are immediately apparent, although a minor disturbance cannot be fully ruled out. The galaxy exhibits a fairly regular shape, being somewhere between perfectly round and elongated.
