The galaxy presents a generally smooth, elliptical morphology. The light is centrally concentrated, with a gradual decline in surface brightness outward from the core. The core exhibits a yellowish hue, which may indicate an older stellar population. There is a faint, diffuse halo surrounding the core, appearing slightly bluer in color. There is no discernable spiral arm structure or dust lane features are observed. The overall symmetry suggests a relaxed system with no current major merger events evident, although there is some very minor possible disturbance in its profile.