The galaxy presents a morphology characterized by a central bulge with an extended, yet ill-defined, disk. The bulge appears to be relatively smooth and concentrated, displaying a yellowish hue, suggestive of an older stellar population. The disk exhibits a bluer color profile, hinting at ongoing star formation.

There is a degree of disturbance in the morphology. The disk is not fully resolved, but appears somewhat irregular. Some regions show a mottled texture, which might indicate clumpy star formation or dust obscuration. There is no obvious sign of a strong bar structure. There are some subtle distortions in the outer regions of the disk, possibly from interactions with a smaller galaxy.
