The galaxy presents as a centrally concentrated, smooth structure with an apparent elliptical morphology. The core exhibits a bright, yellowish hue, which may indicate an older stellar population and/or dust obscuration. The outer regions display a gradual fading of light intensity, with a transition toward redder colors at the edges. There is no discernable spiral arm structure or prominent disk features visible. The overall appearance suggests a relatively undisturbed system, with no clear indications of recent major merger activity. Some minor asymmetry might be present, though the resolution limits definitive assessment.
