The galaxy presents a relatively smooth, elliptical morphology. Its light distribution appears concentrated, with a bright, somewhat diffuse core region indicating a possible active galactic nucleus or a high density of stars. The galaxy appears to be intermediate in roundness. There is a smaller, fainter object located near the galaxy. This could be a smaller galaxy or another object interacting with the galaxy. Overall, the galaxy shows no signs of major disturbance or ongoing merger events, although minor disturbances cannot be ruled out. The color suggests it is a population of older stars, with relatively low levels of ongoing star formation.
