The galaxy presents as a relatively face-on spiral galaxy with a moderate-sized bulge. The spiral arms are readily apparent, displaying a somewhat flocculent structure with a moderate degree of winding. There's some evidence of a possible bar structure across the central region, though it doesn't appear strongly defined. The galaxy color suggests active star formation within the disk, with an overall blueish hue in the arms compared to the yellowish central bulge, potentially indicating older stellar populations there. No major signs of strong interactions or ongoing mergers with another galaxy are visible, though there might be minor asymmetries within the disk indicative of past minor disturbances. There may be 2 to 3 main spiral arms.
