The galaxy presents as an elongated, lenticular-like structure. It displays a smooth, centrally concentrated brightness profile, with a core emitting intensely across the visible spectrum, suggestive of a significant population of older stars, which would have lower star formation. Its disk is oriented close to edge-on relative to our line of sight. The color gradients across the galaxy appear relatively uniform, with a slight bluer cast towards the outer disk and a yellower center. There are only very minor signs of spiral arm structure or dust lanes visible, and no signs of on going mergers, but perhaps minor disturbances. It would be an estimated median mass range for galaxies.
