The galaxy presents as a somewhat elongated, diffuse object. A central, brighter region is apparent, suggesting a concentration of stellar mass towards the galactic nucleus. The galaxy exhibits a generally smooth appearance with minimal evidence of strong spiral arms or distinct morphological features. There is a hint of asymmetry, with one side appearing slightly more extended than the other. The colour profile suggests a mix of stellar populations, with bluer hues concentrated in certain areas, potentially indicating regions of active star formation, and redder hues concentrated in the central region, potentially indicating a population of older stars. Overall, the galaxy appears to be a mid-sized system with an intermediate level of star formation activity and a likely mass on the lower end for galaxies in our universe. There is a subtle indication of disturbance to the morphology, suggesting a minor interaction may have recently occurred.
