The galaxy presents a disk-like structure, viewed at a significant inclination, approaching edge-on. Evidence of spiral arm structure is present, exhibiting a somewhat flocculent morphology. A central bulge is discernible, appearing moderately sized and displaying a yellowish hue, suggesting an older stellar population. A bar-like feature seems to be present, although not prominently defined, extending from the central bulge. The disk itself displays a bluer color profile in the outer regions, suggestive of ongoing star formation. The overall structure indicates a possible disturbance, but no clear signs of an ongoing major merger are observed.
