The galaxy presents a largely smooth, elliptical morphology. There is little indication of spiral arm structure or a prominent disk. The central region exhibits a high surface brightness, appearing nearly spheroidal and quite concentrated. The galaxy appears relatively round, with minimal elongation. There may be slight disturbances visible in the outer regions, suggesting a potential interaction or minor merger history, but it doesn't appear to be a major ongoing merger. The color profile suggests a bias towards older stellar populations, with light tending towards the redder end of the spectrum. This indicates a comparatively low star formation rate at the current time.
