The galaxy appears as a relatively smooth, elliptical-like object. Its color profile suggests an older stellar population, with a dominant yellowish-red hue in the central region, indicating the presence of evolved stars. The overall morphology lacks prominent spiral arms or distinct features typically associated with active star formation. There might be a very faint, diffuse disk-like structure present upon close examination, but it's not clearly defined. The galaxy's shape appears close to circular. There is no obvious evidence of a major merger event or significant tidal disturbances in the galaxy's structure.
