The galaxy presents as a somewhat diffuse, elliptical structure. It appears largely spheroidal in shape with a high degree of central concentration. The galaxy exhibits a generally smooth morphology, lacking obvious spiral arm structures or prominent dust lanes in the available image resolution. The central region of the galaxy shows a subtle color gradient, transitioning from a more yellow-orange hue towards the outer regions to a more red hue. The galaxy appears relatively isolated, with no immediately apparent signs of a major ongoing merger, although some subtle tidal features or minor disturbances cannot be entirely ruled out. The galaxy's estimated half-light radius suggests that the galaxy spans approximately 7.2 kpc. Overall, the galaxy's morphology suggests that it is a relatively quiescent and mature system.
