The galaxy presents a largely smooth morphology, exhibiting a high degree of central concentration. The light distribution indicates a generally elliptical shape, appearing quite rounded, with only a slight deviation from perfect circularity. There's no strong evidence of spiral arm structure or a prominent disk. A reddish hue dominates the central region, possibly indicative of an older stellar population or significant dust obscuration. The outer regions display a color gradient, shifting towards green, which could signify a younger, hotter stellar population in these areas, although faint and not particularly pronounced. Minor disturbances, such as tidal tails or irregular features, are absent. The overall impression is of a relatively undisturbed system, evolving in isolation.
