The galaxy presents an overall disk-like morphology with a central bulge region. The bulge appears primarily yellow-orange in color, suggesting an older stellar population. The disk component appears less organized, with some areas showing bluer hues, possibly indicating regions of ongoing star formation, while other areas are predominantly red, likely containing older stars or dust. There are indications of disturbances in the disk, such as asymmetries or faint tidal features, suggesting that the galaxy may have experienced a past or ongoing interaction with another galaxy, perhaps resulting in a merger.
