The galaxy presents as a moderately luminous, early-type system at a redshift of approximately 0.028. It exhibits a predominantly smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The central bulge is bright and concentrated, transitioning into a more diffuse halo. The galaxy appears nearly round. There is little evidence of recent major merger activity or significant tidal disturbances in its immediate vicinity. Low levels of star formation may be ongoing. Overall, the galaxy's characteristics suggest a relatively evolved system with a substantial stellar mass.
