The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The core exhibits a bright, diffuse glow, suggesting a high density of stars or active galactic nucleus activity. The galaxy does not display a well-defined spiral structure or a prominent disk. Instead, it possesses an extended halo or envelope, which appears somewhat irregular and possibly disturbed. There are hints of faint features or substructures within the halo, indicating potential tidal interactions or past merger events. Color gradients suggest a diverse stellar population. Overall, this galaxy appears to be an evolved system, potentially undergoing or having recently undergone significant gravitational interactions.
