This galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a bright, moderately diffuse core. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly circular shape. There are suggestions of minor disturbances in the overall light distribution, which may be indicative of tidal interactions or internal processes. The color profile is predominantly bluish-white, suggesting a moderate population of younger stars, although the smoothness also suggests an older population. The overall structure seems undisturbed by any recent major mergers, but smaller, lower-level disturbances might be present.
