The galaxy presents as a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge with a noticeable decrease in surface brightness moving outwards from the core. The color profile is generally red-shifted, suggesting an older stellar population, and minimal ongoing star formation. There is no clear evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a well-evolved system, likely a massive galaxy, showing minimal signs of recent interaction or disturbance.
