The galaxy appears as a somewhat smooth, elliptical-like object, exhibiting a concentration of light toward its center. The galaxy's overall color seems to be towards the redder side, which is consistent with an older stellar population, potentially indicating lower levels of ongoing star formation. There is a slight hint of a disk-like structure but it is very indistinct. No major disturbances or signs of ongoing merging are immediately evident, though minor asymmetry cannot be ruled out. The galaxy's apparent round shape is supported by visual examination.
