The galaxy presents as a moderately luminous elliptical galaxy with a smooth, centrally concentrated morphology. There is a slight elongation in its shape, suggesting a possible deviation from perfect sphericity but is more lenticular, showing a disklike feature without strong spiral arm structures. Color gradients are subtle. The core exhibits a warmer color, trending towards yellow-white, which suggests the presence of an older stellar population. The outer regions fade into a more diffuse, redder hue, also indicating a lack of ongoing active star formation in the outer reaches. There is a faint suggestion of a tidal disturbance, perhaps evidence of a recent, minor merger event, although the galaxy appears largely relaxed and settled in its current state.
