The galaxy presents as a fairly symmetrical, elliptical form. There is a concentrated central bulge, a region of increased luminosity indicating a high density of stars. The light profile appears smooth with no clear spiral arm structures visible. The galaxy's color suggests an older stellar population, with a shift toward redder wavelengths. This implies a relatively low rate of active star formation. Minor disturbances may be present, though not markedly disruptive. The overall structure points to a galaxy that is likely undisturbed and well established.
