The galaxy presents as a relatively smooth, lens-shaped structure, with a higher concentration of light toward the center. The overall color appears slightly redder, suggesting a population of older stars. It's elongated, with a possible weak disk shape. There is no apparent merger activity, such as tidal tails or distorted morphology. The galaxy exhibits characteristics that suggest it is not a pure elliptical galaxy, as it has features and signs of rotation that may classify it as lenticular.
