The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. It exhibits a generally round morphology, lacking any prominent spiral arms or bar structures. The light distribution suggests a gradual decrease in intensity from the core outwards, with no distinct features indicating recent major merger events. The galaxy's color profile is somewhat uniform with a tinge of a yellow color, implying an older stellar population and a relatively low rate of ongoing star formation. There are only slight indications of any minor disturbances in the galaxy's structure.
