The object appears to be a galaxy with a somewhat irregular morphology. The central region exhibits a bright, compact core, with a high concentration of blue light, suggesting a population of hot, young stars, or perhaps an active galactic nucleus. There is evidence of extended structure beyond the core, with a slightly elongated shape. Faint, diffuse extensions are present at the periphery. There are possibly very subtle tidal features on either side of the galaxy, though they are very weak and could potentially be artifacts. Overall, the galaxy does not exhibit strong spiral arm structure or a well-defined disk, but seems to be more amorphous.
