The galaxy presents a fuzzy, somewhat irregular morphology. There is evidence of possible tidal features or disturbed structure, though the image resolution limits detailed assessment. The central region appears brighter and more concentrated, suggesting the presence of a galactic nucleus. A subtle disk-like structure might be present, though not clearly defined. Faint extensions or plumes are potentially observed extending from the main body, indicating possible interactions or past merger events. The color distribution within the galaxy indicates a diverse stellar population, with some regions possibly exhibiting younger, bluer stars, while others suggest older, redder populations. Star formation activity appears to be present, though not overwhelmingly dominant. The overall appearance suggests a galaxy undergoing a period of transition or interaction.
