The galaxy presents as a somewhat elliptical, diffuse structure. The central region exhibits a notably brighter, concentrated glow, suggesting a higher density of stars or possibly an active galactic nucleus. The overall color appears to be in the yellowish-orange range, which might indicate an older stellar population with fewer young, hot, blue stars and a higher proportion of red giants and supergiants. There is a slight asymmetry to the shape, possibly indicating a past or ongoing minor gravitational interaction, though the structure appears mostly relaxed. The size suggests it is a substantial galaxy. There are no distinct spiral arms or a prominent disk visible. Any indications of star formation appear relatively subdued.
