The galaxy appears to be a spiral type, though with some irregularities in its morphology. A central bulge is visible, exhibiting a yellow-orange hue. Diffuse spiral arms extend from the bulge, exhibiting a blueish color, indicating the presence of younger, hotter stars and regions of active star formation. There is a clear asymmetry present, suggesting possible interactions or recent mergers, supported by a disturbed shape and possible tidal features. The galaxy's disk does not appear to be well-defined, showing some patchiness and irregularity in the distribution of stellar populations. A possible bar structure might be present at the center of the bulge. Dust lanes are difficult to discern, but there are some dark regions within the spiral arms that may indicate the presence of obscuring dust. The overall structure hints at a system undergoing dynamic changes, potentially due to ongoing interactions with neighboring galaxies.
