This galaxy presents a largely smooth, elliptical morphology. It appears highly concentrated with a bright, well-defined nucleus. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests an older stellar population, with a central region exhibiting a yellow-orange hue, potentially indicating a dominance of evolved stars. The outer regions fade into a slightly bluer color, possibly due to the presence of a small number of younger stars. No indications of major merging events or tidal disturbances are apparent.
