The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated luminosity profile. There is a distinct lack of spiral arm structures or prominent dust lanes. The overall color is bluish-white, suggesting the presence of a moderate population of young, hot stars, although the smoothness indicates a lack of widespread active star formation. There may be a subtle, minor disturbance present in the morphology, hinting at a possible past interaction or minor merger event, although the main body of the galaxy remains relatively undisturbed. The galaxy does not appear to be perfectly spherical; there is a slight elongation. There is some evidence of a faint outer halo or extended stellar population surrounding the main body, though it is diffuse and not well-defined.
