The galaxy appears as a slightly elongated, diffuse object with a relatively smooth light distribution. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a bulge. A subtle color gradient is observed, with the central bulge appearing slightly yellower compared to the outer regions, hinting at a potential difference in stellar populations, with older stars residing in the bulge. There are no prominent spiral arm structures visible, nor any strong evidence of recent major merger events. The overall morphology suggests a classification toward the elliptical or lenticular side, with only minor disturbances, implying it has reached a more evolved state.
