The galaxy appears to be a luminous, elliptical system exhibiting a relatively smooth morphology. The central bulge is quite prominent and appears nearly spherical. There is a slight elongation to the overall structure, which suggests a deviation from perfect circularity. The light profile transitions smoothly from the bright core to the fainter outer regions, without any obvious spiral arm structures or dust lanes. There is some faint and diffuse halo surrounding the central region. While there are no distinct features indicating a major interaction or ongoing merger, there is potentially some minor disturbance to the overall symmetrical structure of the galaxy. The galaxy's color index suggests a population of older stars.
