The galaxy presents a morphology characterized by a dominant central bulge, surrounded by a fainter disk component. The bulge exhibits a smooth, featureless appearance, suggesting an older stellar population. The disk, while present, appears somewhat disturbed, with a fuzzy, irregular structure and a lack of well-defined spiral arms. A significant portion of the galaxy's light appears concentrated in the bulge. The galaxy exhibits a noticeable color gradient, with a more yellow-orange hue in the central region and a bluer tint in the outer regions of the disk. There is a possible tidal feature or merging companion.
