The galaxy presents a largely smooth, elliptical morphology, displaying a high degree of central concentration. Its color profile suggests an older stellar population, with a notable absence of significant blue light indicative of ongoing, widespread star formation. There is a slight asymmetry.

Given its apparent size, the galaxy is likely relatively massive, and the smoothness suggests it is a evolved system that has largely completed its major mergers, without a recent significant interaction. There are minor signs of disturbance, indicating a possible recent encounter, although not an ongoing merger. The galaxy does not appear to be a disk galaxy from this angle.

