The galaxy presents as a moderately inclined disk galaxy with a prominent central bulge. The bulge appears relatively smooth and concentrated, exhibiting a bright, slightly off-center core. The disk component shows subtle indications of spiral structure, with hints of faint, diffuse arms extending from the bulge. The overall color is somewhat bluer than the bulge, particularly in the outer regions, suggesting the presence of younger stellar populations. The galaxy exhibits a moderate degree of flattening and a slightly elliptical shape. There appears to be some minor asymmetry in the disk, possibly indicating a gravitational interaction or recent merger event.
