The galaxy presents a largely smooth, elliptical morphology, with an apparent red hue suggesting an older stellar population. It appears largely spheroidal, though subtle deviations from perfect roundness suggest a possible, slight disklike structure or ongoing gravitational interaction. There is some asymmetry present in the galaxy's light distribution, potentially indicative of minor disturbances. The concentration of light towards the center is substantial, marking a well-defined galactic nucleus. There is faint surrounding diffuse light that gives a hint of a larger galactic radius. Possible tidal feature to the left.
