The galaxy exhibits a predominantly smooth morphology, appearing as an elliptical or lenticular structure when observed in this photometric band. There is a slight flattening of the galaxy along its major axis, with a bulge, but a smooth, featureless appearance otherwise. The central region exhibits a concentrated brightness, suggesting a significant stellar density or a possible active galactic nucleus. There may be a hint of a disk structure, however this is minor, and it is a centrally concentrated and red galaxy. There is no strong evidence of tidal disturbances or major merger activity. The galaxy's light distribution appears largely symmetrical.