The galaxy presents as a slightly inclined disk galaxy. A prominent central bulge is visible, and seems to dominate the overall light profile. There is also a bright bar of stars cutting across the galaxy’s central region. The disk component appears relatively smooth, and spiral arm structure is not clearly defined, though hints of asymmetry may be present in the outer disk regions. The overall color suggests an intermediate age stellar population. The galaxy appears undisturbed, with no obvious signs of major mergers or tidal interactions. 
