The galaxy presents as a dominant, relatively smooth, elliptical or lenticular structure. Its color appears to be primarily yellow/orange, indicative of an older stellar population with less ongoing star formation. The light distribution is centrally concentrated. There is only a slight hint of a disk-like structure. No obvious spiral arms are visible. A small fraction of the galaxy appears to be experiencing disturbances, suggestive of a potential minor merger event in its past, but it is predominantly a single entity, not showing strong signs of ongoing interaction. It appears to be a relatively massive galaxy with a diameter in the range of approximately 8 kiloparsecs.
