The galaxy presents a flattened, disk-like structure, indicating a likely spiral morphology. Faint spiral arms are visible, appearing somewhat tightly wound and exhibiting a two-armed structure. These arms display a bluer color, suggesting the presence of active star formation. The central bulge is moderately prominent, with a yellow hue indicating an older stellar population. No bar structure is immediately apparent. There are signs of potential minor disturbances, possibly interactions with other galaxies. The galaxy does not appear to be undergoing a major merging event but shows subtle asymmetric features. The overall color gradient suggests a radial distribution of stellar populations, with younger stars concentrated in the arms and older stars dominating the bulge. The observed features indicate the galaxy is relatively far away.
