The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall color is yellowish-orange. The central bulge is bright and somewhat diffuse, surrounded by a fainter, more extended halo or disk component. There is a hint of a flattened structure, but no clear spiral arms or strong dust lanes are visible. The overall appearance suggests a galaxy with a significant population of older stars and a relatively low rate of on-going star formation. There may be some minor asymmetries or irregularities in the outer regions, potentially indicating a past interaction or minor disturbance.
