The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical, appearing nearly round. The light profile exhibits a strong peak at the core, suggesting a significant concentration of stars towards the center, possibly indicative of a supermassive black hole. The galaxy appears primarily yellow-red in color, which suggests a stellar population dominated by older, redder stars with low rates of star formation. There is little evidence of spiral arms or significant dust lanes. There may be a faint and diffuse halo surrounding the central region, though the signal is weak. The galaxy shows no signs of recent major merging events. Small disturbances may or may not be present upon closer inspection.
