The galaxy appears relatively small, exhibiting a slightly elongated shape on the plane of the sky. A subtle central bulge is visible, with faint spiral arm features extending outwards. These arms appear somewhat disrupted or irregular. There may be indications of tidal disturbances or interactions with other galaxies. Patches of blueish light, likely indicating regions of recent star formation, are visible in the arms. The overall color suggests a mixed stellar population, with a combination of older, redder stars in the bulge and younger, bluer stars in the spiral arms. A minor merger or close interaction cannot be ruled out based on morphological features.
