The galaxy presents a discernible disk structure, viewed at a slight inclination to our line of sight. Spiral arm features appear somewhat flocculent and are not sharply defined, though the overall structure suggests a spiral morphology. A central bulge region is evident, exhibiting a moderate size relative to the overall galactic disk. The bulge appears relatively smooth and intensely bright, exhibiting a yellow-white coloration, potentially indicative of a population of older stars. The disk component displays bluer hues, likely a result of ongoing star formation activity. The presence of a bar-like structure can be tentatively identified. There is no obvious indication of tidal disturbances or ongoing major merger events. The overall morphology suggests this is an intermediate spiral galaxy with a notable bulge and moderate star formation within the disk.
