The galaxy presents a moderately inclined, disk-like structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Surrounding the bulge, the disk displays a bluer color, which could indicate more recent star formation within the disk. Some asymmetries can be observed throughout the disk, indicating some form of gravitational disturbance. Overall, the disk appears relatively smooth, without prominent spiral arm structures. However, there's a subtle suggestion of faint, diffuse features emerging from the central region. The galaxy appears relatively isolated. 
