The galaxy appears as a relatively small, disk-shaped system, presenting an edge-on or highly inclined orientation relative to the observer's line of sight. There is a central bulge that has a brighter, more concentrated luminosity profile. The bulge exhibits a blue-green hue, suggesting a population of younger, hotter stars or significant ongoing star formation. 

Extending outwards from the central bulge, a fainter, flattened disk structure can be observed. This disk also has a blue-green coloration, consistent with the central bulge and indicative of active star formation. There is a slight asymmetry in the distribution of light within the disk, possibly from a minor disturbance. Some redness is visible closer to the galactic center.

Overall, the galaxy appears to be actively forming stars. The disk appears relatively smooth but with a minor disturbance in morphology.
