The galaxy appears as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, indicating a prominent nucleus or bulge. The overall color profile suggests a relatively old stellar population, with a dominant yellowish-red hue. There is little evidence of ongoing star formation, as indicated by the lack of bright blue regions typically associated with younger, hotter stars. There is no dust apparent in the image. It does not appear to be undergoing a major merger, or have any large disturbances in its overall structure. It looks to be a relatively settled galaxy.
