This galaxy presents as a relatively compact, disk-like structure exhibiting a blue hue, suggesting the presence of a younger stellar population and ongoing star formation. The central region displays a slightly brighter, concentrated luminosity, possibly indicating the presence of a galactic bulge. While a distinct spiral arm structure is not immediately apparent, there are hints of irregular features and subtle distortions in the disk, indicating possible tidal interactions or minor merger events in its recent history. The overall appearance suggests a moderate level of disturbance. The galaxy is relatively small, and it appears that at least some amount of star formation is ongoing within its disk. 
