The galaxy presents a largely smooth, elliptical morphology. It is a well-defined object with a centrally concentrated luminosity profile that diminishes gradually outwards. The primary body of the galaxy is nearly round, but appears slightly elongated along one axis. There is little evidence of spiral arm structure or strong dust lanes.

The galaxy exhibits a color gradient, appearing more yellowish in the central region and transitioning towards bluer hues in the outer parts. The moderate level of blue light in the outer regions suggests the presence of a young stellar population, which implies ongoing or recent star formation, albeit at a relatively low rate. Faint irregularities are present, suggesting either a minor interaction with another galaxy or internal disturbances. A small portion shows signs of a disrupted morphology. The stellar mass is substantial.
