The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. Its color profile is predominantly yellow-red, suggesting an older stellar population with a relatively low rate of ongoing star formation. The galaxy exhibits high degree of roundness in shape. There is no apparent spiral arm structure or significant dust lane obscuration visible. Minor disturbances are potentially visible, possibly indicating past interactions, though a major merger event is unlikely. The overall morphology suggests it is an early-type galaxy, possibly a massive elliptical at a considerable distance.
