The galaxy presents a somewhat flattened, disk-like morphology. The central region exhibits a bright, concentrated bulge, appearing relatively smooth in texture and showing a yellowish hue, suggestive of an older stellar population. Extending outwards from the bulge, the disk demonstrates a mottled appearance, indicative of some degree of substructure. 

There is evidence of possible spiral arm structures. These arms are faint and somewhat irregular. The overall color of the disk is bluer than the bulge, implying a more active star formation rate within the disk.

There appears to be evidence of a potential minor disturbance in the morphology of the galaxy, possibly a slight asymmetry or warped feature in the outer disk. This may be indicative of a past or ongoing minor merger event. The galaxy is oriented close to edge-on.
