The object appears to be a spiral galaxy viewed nearly edge-on. The galaxy exhibits a prominent, flattened disk structure. There is a bright central bulge, and is more luminous and potentially comprised of a higher density of older stellar populations. The disk appears relatively smooth, with little to no visible arm structure. The galaxy lacks any obvious signs of recent merger activity or strong gravitational disturbances. The light from the galaxy appears reddish. Its morphology suggests ongoing star formation, but is overall a relatively quiescent galaxy with a redder color index.
