The galaxy presents a generally elliptical morphology, with a smooth and concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arm structures or distinct features typically associated with active star formation regions. The galaxy exhibits a slight elongation, its shape being neither perfectly circular nor highly flattened. The overall color profile suggests a composition dominated by older stellar populations, with a higher concentration of redder light emanating from the bulge compared to the outer regions. There is some evidence of a subtle color gradient, transitioning towards bluer hues in the outskirts, which could indicate the presence of younger stars or a lower metallicity environment away from the galactic center. No signs of a major ongoing merger event are discernible, although subtle disturbances or tidal features in the outermost regions cannot be entirely ruled out without more detailed analysis.
