The galaxy presents as a somewhat amorphous structure, displaying an irregular morphology rather than a well-defined spiral or elliptical form. There is evidence of possible tidal features or disturbances in the structure of the galaxy. These disturbances possibly imply interactions or past merger events with other galaxies, disrupting its original form. The central region of the galaxy appears more concentrated and brighter, suggesting a higher density of stars or an active galactic nucleus, although the image resolution limits definitive conclusions. There are areas of redder hue, which may indicate regions of dust obscuration or older stellar populations. The distribution of light is uneven, indicating a complex interplay of star formation, dust extinction, and stellar populations within the galaxy. Overall, the galaxy seems to be in a dynamically active state, experiencing interactions or other processes influencing its structure and star formation activity.
