The galaxy appears to be a luminous elliptical galaxy with a relatively smooth morphology. Its shape is moderately elliptical, leaning towards round rather than elongated. The core exhibits a reddish-orange hue, potentially indicating an older stellar population or dust obscuration, while the outer regions appear slightly bluer, hinting at some ongoing star formation, though not particularly vigorous. There may be a minor disturbance present in the structure, though this is difficult to ascertain definitively due to the spatial resolution. There is no obvious presence of spiral arms or a well-defined disk. The galaxy is relatively massive and demonstrates moderate star formation.
