The galaxy presents as a faint, extended object with a slightly elongated morphology. A central bulge is evident, appearing relatively smooth and concentrated. The surrounding disk exhibits a mottled texture, hinting at potential spiral arm structures, though they are not sharply defined. The color distribution suggests a population of older stars concentrated in the bulge, indicated by the yellow-red hue, while the bluer tones in the disk may signify ongoing or recent star formation. There is a subtle asymmetry in the outer regions, possibly indicating a minor gravitational interaction or tidal disturbance. Overall, the galaxy appears to be a disk galaxy, viewed at a slight angle from edge-on.
