The galaxy appears as a moderately bright, somewhat diffuse object with an overall elliptical morphology. The light distribution is relatively smooth, suggesting a dominance of older stellar populations. There is a subtle elongation, but the galaxy is mostly round in shape. A slight asymmetry is visible, potentially indicative of a minor tidal interaction or recent accretion event. The lack of distinct spiral arm structures suggests that the galaxy is an early-type galaxy. There is a suggestion of a small amount of on-going star formation. The galaxy is likely a relatively massive system, given its overall brightness and extent. There is a faint, diffuse halo surrounding the main body of the galaxy.
