The galaxy appears to be a single, centrally concentrated object. Its overall morphology is smooth, with a generally elliptical shape that is slightly elongated. There is a noticeable color gradient, transitioning from a warmer, yellower core to a slightly cooler, more red-tinged outer region. Though the central region appears relatively homogenous, there is an indication of potential disturbance in the galaxy morphology. There appears to be some low level merging occurring, although no major signs of disturbance, like a tidal tail, is present. The central bulge dominates the appearance, with little evidence of a prominent disk structure. Overall, the galaxy exhibits characteristics consistent with a fairly massive system undergoing active star formation, with relatively low amounts of dust.
