The galaxy presents as a centrally concentrated, smooth structure, likely an early-type system. Its overall shape is elliptical. There is a slight elongation, although the galaxy is mostly rounded. No distinct spiral arm features are visible, nor are there apparent signs of a recent or ongoing major merger. It appears largely undisturbed. The color profile suggests a relatively evolved stellar population, likely consisting of older, redder stars. There may be indications of ongoing star formation activity, given the blue tint in the center, but it is likely at a low rate.
