The galaxy presents as a moderately elliptical object with a smooth, diffuse morphology. The central region appears bright and concentrated, suggestive of a prominent galactic nucleus. There are no distinct spiral arms or bar structures visible. The overall color profile indicates a population of stars that are largely intermediate to old in age. The gradient in color from the core to the outer regions is subtle, though it appears that the core is somewhat redder than the areas surrounding it. There is no obvious evidence of significant dust lanes or ongoing star formation regions, although the bluer light surrounding the core suggests that some ongoing star formation may exist at some level.
