This galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth and somewhat rounded, although there is visible irregularity in its form. Emanating from this central region are faint extensions of light, suggesting tidal tails or disrupted spiral arms. The overall color profile appears to be a gradient from a slightly blue hue in regions outside the central region, towards a more reddish color, with a yellow core. The galaxy's structure seems to display significant disturbance, consistent with interactions with another galaxy or a prior merger event that has not yet fully relaxed into a stable configuration. Further spectroscopic analysis would be necessary to fully characterize the dynamics and stellar populations within this galaxy.
