The galaxy appears as a primarily elliptical or lenticular system, exhibiting a smooth, concentrated light profile. The core region is bright and dominates the overall luminosity. There is some subtle indication of a flattened disk-like structure, but it is not pronounced. The galaxy presents a generally round appearance. There is no strong evidence of major mergers or significant tidal disturbances in the immediate vicinity, though subtle asymmetries suggest the possibility of past minor interactions. Considering a redshift of approximately 0.19, the galaxy is relatively distant. The object's color indices suggest that there are older stellar populations and a low rate of current star formation activity. The galaxy's overall magnitude indicates a luminous, massive system.
