The galaxy appears to be a disk galaxy, viewed at an oblique angle, between edge-on and face-on. The central bulge is prominent and relatively smooth, appearing elliptical in shape. A faint disk is visible extending beyond the bulge, exhibiting a bluer hue compared to the central region, suggesting the presence of younger stellar populations. The overall shape is somewhat elongated, indicating a degree of flattening. There are hints of faint spiral arm structures within the disk, though they are not sharply defined. The galaxy exhibits a concentration of light towards the center, with a gradual decrease in brightness moving outwards into the disk. There may be some minor irregularities or disturbances in the outer disk region. Overall, it seems to be a spiral galaxy with a well-defined bulge and a less pronounced or disturbed disk.
