The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, with little to no visible spiral arm structure. The light distribution is centrally concentrated, showing a gradual decrease in luminosity from the core outwards. The color appears relatively uniform across the galaxy, suggesting a generally older stellar population with little ongoing star formation. There is a potential companion or merging object nearby the main galaxy. There may be some tidal disturbances that are not immediately obvious, but warrant closer inspection.
