The galaxy presents a generally smooth, rounded morphology. The central region exhibits a bright, concentrated luminosity, suggestive of a prominent galactic nucleus. There is a gradual decrease in brightness from the core outwards. Faint extensions of light are visible in the outer regions, but there are no obvious spiral arm structures or bar features. There is no evidence of any on going major merger, tidal tails, or strong gravitational distortions in the immediate vicinity of the galaxy. The color appears to be on the redder side, suggesting the stellar population is older.
