The object presents as an elliptical galaxy, with a relatively smooth, though slightly diffuse, light distribution. There is a bright, concentrated core region that appears slightly offset from the overall galactic structure. The main body of the galaxy shows a noticeable flattening and elongation. There is evidence of a faint, diffuse halo extending beyond the main body of the galaxy. Some minor disturbances or asymmetries can be observed in the outskirts of the object, potentially suggesting gravitational interactions. The galaxy's color index suggests a population of older stars. There might be some low-level ongoing star formation indicated by bluer patches. Overall, this galaxy appears to be undergoing some form of dynamic evolution.
