The galaxy presents a somewhat elliptical morphology, suggesting a disk galaxy viewed at an oblique angle, but not quite edge-on. The central bulge is prominent and exhibits a yellowish hue, which may indicate an older stellar population. Fainter, bluer regions extend outwards from the central bulge along the disk, indicating the presence of some ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity. The overall structure suggests a spiral or lenticular galaxy with a relatively smooth appearance.
