The galaxy appears as a relatively small, moderately bright object with a slightly elongated morphology. The core exhibits a high degree of luminosity, suggesting a concentration of stars and potentially an active galactic nucleus. The color profile indicates a bluer hue towards the central region, transitioning to redder tones in the outer edges of the galaxy. This suggests active star formation occurring in the core, while older stellar populations dominate the periphery. There is a hint of irregularity in the galaxy's overall shape, which may indicate some past interaction or disturbance, however its difficult to know for sure.
