The galaxy presents as a centrally concentrated object with a generally smooth appearance. It has an elliptical, nearly circular shape. There is no obvious spiral arm structure. A distinct color gradient is observed from the center outwards. The core appears slightly brighter and bluer in color compared to the outer regions, which exhibit a more yellow-red hue. This suggests a possible presence of a relatively young stellar population in the central region. No obvious tidal tails or signs of a major ongoing merger are apparent, although some slight asymmetry may suggest a minor gravitational interaction or disturbance.
