The galaxy presents a flattened, disk-like morphology, with a moderate inclination relative to the observer's line of sight. A bright, concentrated central bulge is apparent, exhibiting a yellowish hue suggestive of an older stellar population. The surrounding disk shows a bluer color gradient, particularly towards the outer regions. There is evidence of potential spiral arm structure within the disk, although it is somewhat diffuse and not sharply defined. Faint, reddish areas are scattered within the disk, these may indicate regions of ongoing star formation or dust obscuration. There are no obvious signs of strong tidal disturbances or major mergers.
