The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a bright, concentrated bulge that appears to be the dominant feature. The overall shape is not perfectly round, showing a slight elongation.

A faint disk component might be present but is not well-defined. There is no clear evidence of spiral arms or significant star-forming regions directly visible within the main body of the galaxy. The color gradients suggest a population of older stars, with the central bulge exhibiting a redder hue and the outer regions slightly bluer.

There is no obvious sign of a major ongoing merger, though subtle disturbances cannot be ruled out.
