The galaxy presents as a somewhat elliptical structure, appearing largely smooth and featureless across its visible extent. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness outwards. There is a slight elongation, though the overall shape is closer to circular than highly elongated. There is a hint of a disk, but this appears very faint and is close to the bulge. The color gradient is subtle, transitioning from a yellowish core, indicating older stellar populations, to slightly bluer colors in the outer regions, possibly indicative of ongoing, albeit limited, star formation. There is no clear evidence of strong spiral arms or any major merger events. The overall morphology suggests a transition object with a small amount of recent or continuous star formation, but dominated by an old and evolved stellar population.
