The galaxy appears to be a relatively smooth, elliptical galaxy, potentially of type E3-E5. The light distribution suggests a centrally concentrated structure with a radial decrease in surface brightness. The core exhibits a yellowish hue, indicative of an older stellar population with a lower rate of star formation. The outer regions display a slightly bluer color compared to the core, perhaps indicating the presence of a younger stellar population, although the overall color suggests it is not vigorously star-forming. The galaxy is largely devoid of prominent spiral arms or distinct features, and its shape appears slightly elongated. There is no strong evidence of a recent or ongoing major merger event, although some minor disturbances cannot be ruled out with this image resolution.
