This galaxy exhibits a predominantly disk-like morphology with a prominent central bulge. The galaxy is viewed at an oblique angle, suggesting it is not a face-on spiral galaxy. The central bulge appears bright and relatively smooth in texture, indicating a concentration of older stellar populations. A distinct disk component is visible, characterized by a mottled texture suggestive of spiral arms or dust lanes. The color gradient across the disk, with bluer hues in the outer regions, implies ongoing star formation. Faint, diffuse extensions are observed at the edges of the galaxy, possibly indicating tidal features or minor disturbances due to gravitational interactions. The overall structure shows some asymmetry, potentially suggestive of a recent or ongoing minor merger event.
