The galaxy presents as a disk-shaped structure, with a central bulge that appears relatively prominent. The bulge exhibits a yellowish hue, suggesting an older stellar population. The surrounding disk shows a bluer color, indicative of ongoing star formation. There is evidence of spiral arm structure, but it is not clearly defined and appears somewhat patchy. Some irregularities are observed in the outer regions of the disk, possibly due to gravitational interactions or past merger events. The overall morphology leans towards a spiral galaxy, though potentially one that has experienced some form of disturbance. The light distribution is somewhat diffuse, suggesting a moderate degree of dust obscuration.
