The galaxy appears as a centrally concentrated, elliptical-like object. Its core exhibits a bright, yellowish-white color, indicating a potentially older stellar population. The outer regions display a slightly bluer hue, which might suggest the presence of some younger stars or ongoing star formation, albeit at a lower rate. There are no discernable spiral arms or a prominent disk structure, and the overall form seems rather smooth. Slight asymmetry can be observed in the galaxy's outer reaches, suggesting the possibility of a previous minor interaction or disturbance, but without major signs of an ongoing merger event.
