The galaxy appears as a somewhat flattened, disk-like structure. It exhibits a central concentration of light, indicative of a bulge or core region. Surrounding the core is a fainter, extended halo of light. The galaxy displays a color gradient, with the core showing bluer hues, potentially suggesting ongoing star formation. The outer regions are dominated by redder colors indicating a population of older stars. There is a faint indication of spiral arms or irregularities in the disk but the resolution is not high enough to confirm. Based on its morphology, this galaxy could be classified as a spiral or lenticular galaxy. There may be some minor disturbances in the morphology suggesting that the galaxy has been subjected to some tidal interactions. 
