The galaxy presents a flattened, disk-like morphology, viewed at a moderate inclination. It exhibits a noticeable central bulge that is relatively bright and concentrated, surrounded by a fainter, more diffuse disk. The overall color appears to be yellowish-white, suggesting an older stellar population with reduced ongoing star formation. The spiral arm structure, if present, is not clearly defined in this image, indicating either tightly wound arms or a lack of prominent star-forming regions that would otherwise highlight the spiral pattern. There are no obvious signs of major mergers or significant tidal disturbances within the galaxy's immediate structure. It appears relatively undisturbed, indicative of a system evolving in a relatively isolated environment.
