The galaxy appears to be a late-stage spiral or an irregular type. A distinct disk structure is not readily apparent, though there are indications of a slight flattening. The light distribution is not smooth, and the galaxy shows some lumpy features. Possible faint tidal tails or distorted arms are seen along the right edge of the image, which could be indicative of a recent or ongoing merger event. Color gradients are evident, with the central region showing a slightly redder hue compared to the outer regions, implying a more aged stellar population toward the core. There is evidence of possible dust lanes or regions of obscuration contributing to the irregularity of the light distribution. The object presents an overall disturbed morphology.
