This galaxy appears to be an interacting system undergoing some type of disturbance. The core of the galaxy exhibits a bright, concentrated central region, suggestive of a potential active galactic nucleus or a region of intense star formation. The galaxy appears to be surrounded by a faint, diffuse halo, possibly composed of stellar populations ejected during a gravitational interaction.

Visually, the galaxy does not show any clear spiral arms. Instead, there is some asymmetric structure, especially on the left side of the image, that could be tidal tails resulting from an ongoing interaction with another galaxy or a past merger event. The overall color of the galaxy seems to vary, with the central regions appearing bluer.
