The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, suggesting a significant stellar population density. A gradual decrease in brightness is observed moving outward from the core. There is no apparent spiral arm structure. The overall color of the galaxy appears relatively red, indicative of an older stellar population with low ongoing star formation. There is some slight evidence of a minor disturbance in the galaxy's morphology, potentially indicating a recent or ongoing minor merger event. The shape is generally round, with a very slight deviation toward a more elongated form.
