This galaxy appears to be a relatively smooth elliptical or lenticular type. The light distribution suggests a high degree of spherical symmetry, with a centrally concentrated bulge region. There are no clear spiral arms or bar-like structures visible. The color profile indicates an older stellar population. The galaxy appears slightly disturbed with some possible minor tidal features. These are indicated by slight asymmetry in the outer halo and a possible faint tail-like structure, suggesting a past interaction with another galaxy. Overall, the galaxy seems to be relatively mature.
