The galaxy appears to be a relatively bright, disk-shaped object with a notable central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population with minimal ongoing star formation. Moving outward from the bulge, the disk presents a more complex color profile. There's a mottled appearance with regions of bluish-white interspersed with areas of redder light. This implies a combination of younger, hotter stars concentrated in some regions, likely associated with active star formation, and older, redder stars elsewhere.

The galaxy does not present a clear spiral arm structure. There is some asymmetry and faint filamentary structures in the outer regions of the disk. There is no clearly defined central bar. The overall form appears to be more like a disk galaxy with some irregularities, possibly indicating recent or ongoing interactions or internal dynamic processes. The galaxy is not perfectly symmetrical. This observation implies that the morphological classification leans towards a disk galaxy with a significant bulge and some degree of disturbance.
