The galaxy presents as a predominantly smooth, centrally concentrated object with an elliptical morphology. The color profile suggests a relatively evolved stellar population, indicated by the redder hue observed in the optical bands. There is a distinct yellow/orange bulge, which is characteristic of older star populations. The galaxy's isophotes appear mostly regular. While a slight asymmetry is noted, there is no strong indication of any disk-like structure. The object's form is mostly regular, and there is no strong evidence of any tidal disturbances. It is likely a massive galaxy with little star formation occurring within it.
