The galaxy appears to be a spiral galaxy, although somewhat disturbed or irregular in form. A faint but noticeable disk structure is visible. The galaxy exhibits a central bulge, though not particularly prominent. The disk shows evidence of spiral arm structure, with some indications of ongoing star formation regions within the arms, noticeable as brighter, bluer knots. There is some asymmetry present in the overall shape and distribution of light, possibly indicating a past or ongoing interaction or merger event. The galaxy's light distribution is relatively smooth, consistent with a Sersic profile, but the irregular features suggest a more complex morphology. The disk is not perfectly edge-on or face-on, being tilted at an angle.
