The galaxy presents as an elongated, disk-like structure, viewed nearly edge-on. There is a prominent central bulge that appears relatively smooth and concentrated. Fainter, diffuse light extends outwards from the bulge, forming a flattened disk. The disk exhibits a subtle colour gradient, transitioning from a yellowish hue towards the bulge to slightly bluer tones at the outer edges. No distinct spiral arm features are discernible; instead, the disk appears largely smooth, potentially indicating a lack of significant ongoing star formation. There is no apparent evidence of a major merger, though some minor disturbances cannot be ruled out based on the asymmetry in its disk. The overall morphology suggests a galaxy of substantial mass with a moderate rate of star formation.
