The galaxy presents as a generally smooth and centrally concentrated light source. The color gradient suggests an aging stellar population, trending towards redder hues in the central bulge. The galaxy exhibits a slight elongation, appearing elliptical in shape. No distinct spiral arm structures or prominent dust lanes are readily observable. There is a subtle indication of a faint, extended halo or disk surrounding the bright central region. The relative smoothness of the galaxy indicates it has not undergone any major recent mergers.
