The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The luminosity distribution appears relatively even, with a gradual decrease in intensity from the center outwards. The galaxy's color profile suggests an older stellar population, with a yellow-red hue indicative of lower levels of recent star formation. There is a very slight visual asymmetry to the object suggesting possible gravitational interactions, however this may just be dust obscuration. The galaxy exhibits a moderate angular size, hinting at a substantial physical extent when considering its likely distance.
