The galaxy presents a generally smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish-white hue suggesting a population of older stars. Moving outwards from the core, the galaxy's light gradually diminishes, with a transition towards a slightly redder, more diffuse halo. There is a subtle disk-like feature that can be observed. Its shape is not perfectly spherical, it has a slight cigar shape. No strong signs of recent or ongoing major merger events are evident, although there may be some minor structural disturbances or faint tidal features hinting at a past interaction, primarily on the outskirts of the galaxy. Star formation appears to be relatively quiescent, with a low rate, based on the subdued blue colors in the outer regions.
