The galaxy presents a morphology consistent with a spiral type. The central bulge appears prominent and exhibits a smooth, concentrated distribution of light, suggestive of an older stellar population. Surrounding the bulge, faint, diffuse arms extend outwards. These arms display a mottled texture, indicating regions of star formation. The colour gradient shifts from a yellowish hue in the central bulge to bluer tones in the arms, possibly due to younger, hotter stars. The overall structure exhibits some level of asymmetry, with hints of a minor disturbance in the disk.
