The galaxy presents as a centrally concentrated, generally smooth object with a slightly round morphology. There is no significant evidence of a disk structure or spiral arms within this visual representation. The light distribution suggests that the bulge component is a more prominent feature. The color profile suggests it's primarily in the blue/green range, indicative of moderate ongoing star formation. There is very slight asymmetry to the galactic structure which can be indicative of a possible minor disturbance or past interaction. No signs of merging or a major disturbance.
