The galaxy presents a diffuse, somewhat elliptical morphology. It exhibits a smooth appearance, with no prominent spiral arms or distinct features immediately apparent. The light distribution is centrally concentrated, fading gradually towards the outer edges. There might be a very subtle disk-like structure, but it is difficult to determine without more detailed analysis. The galaxy's color appears relatively uniform across its extent, suggesting a consistent stellar population or dust distribution. There is no strong evidence of any major ongoing merger activity, although subtle disturbances cannot be ruled out. The galaxy is oriented at an intermediate angle to our line of sight.
