The galaxy presents a generally smooth, elliptical morphology with a relatively high degree of central concentration. There is no strong evidence of spiral arm structure or a prominent disk component. The light distribution appears roughly rounded. The galaxy exhibits a subtle color gradient, appearing slightly bluer in the central region and gradually reddening towards the outer regions. The galaxy does not appear to be strongly interacting with any other galaxies. The central light is compact and well-defined. The overall color suggests a population dominated by older stars.
