The galaxy appears to be a relatively smooth, elliptical-like object. It exhibits a bright, concentrated central region, suggesting a significant bulge component. The overall color is bluish-white, indicative of a population of younger, hotter stars within at least some portion of the galaxy. There's no obvious spiral arm structure visible, but there are faint, slightly extended features that could possibly suggest a very faint disk. There are no obvious signs of major mergers or strong tidal disturbances, although subtle irregularities could hint at minor interactions. The galaxy exhibits a modest size, and its color suggest ongoing star formation.
