The galaxy appears to be an edge-on spiral or lenticular galaxy. Its morphology suggests a relatively smooth structure, though with some evidence of internal features. A slight distortion in the shape hints at possible interactions or past mergers. The galaxy exhibits a colour gradient, from a bluer tint at its edges to a redder hue toward the central bulge. This suggests a difference in stellar population, with younger, hotter stars populating the disk and older, cooler stars concentrated in the bulge. There are no clear spiral arm structures visible, but the colour distribution suggests some ongoing, albeit moderate, star formation activity. The elongation is quite high which is also consistent with a galaxy undergoing a tidal interaction or merger.
