The galaxy presents as an edge-on spiral, exhibiting a highly flattened disk structure. A prominent central bulge is observed, displaying a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluer regions extend along the outer edges of the disk, potentially indicating areas of active star formation within the spiral arms. The dust lane appears prominent, obscuring some of the light from the bulge. No significant tidal features or indications of a major merger event are visually apparent. The galaxy shows a relatively smooth morphology, with only slight disturbances visible, suggesting a quiescent state. The bulge appears to be rather boxy.
