The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated bulge. There is a slightly elongated shape, not perfectly spherical but leaning towards a more oblong form. The light profile suggests a fairly evolved system, with a dominance of older stellar populations, indicated by the reddish-yellow hue in the central region. The outer regions display a slightly bluer tint, perhaps suggestive of some ongoing, although likely subdued, star formation activity within the disk. The galaxy may be undergoing a minor merger with another galaxy or experiencing some tidal disturbance, as it may appear to be an asymmetric structure.
