The galaxy presents as an elongated, disk-like structure, observed at an oblique angle, but not quite edge-on. There is a central, brighter region indicative of a galactic bulge or a concentration of older stars. The disk shows a mottled appearance, with subtle variations in color and brightness, suggesting areas of star formation or dust obscuration. The overall color of the galaxy appears to be slightly blue-tinged, possibly indicating a moderate level of ongoing star formation. There is a faint, diffuse halo of light surrounding the main disk, suggesting the presence of a stellar halo. No distinct spiral arm structures are clearly visible, though there may be subtle hints of features within the disk. There is no prominent bar structure detected. The general morphology points to a galaxy that is neither a pure elliptical nor a well-defined spiral, but rather a disk galaxy with some characteristics of both.
