This galaxy presents as a merging system or a galaxy undergoing a major disturbance. The morphology suggests at least two distinct nuclei, exhibiting a luminous, yellowish glow, indicating a population of older stars within the central regions. The overall shape is irregular, with an elongated structure suggesting tidal forces are actively reshaping the galaxy. Faint extensions of light are observable, potentially indicative of tidal tails resulting from gravitational interactions. These are reddish in hue and have a smooth texture. The surrounding halo presents a greenish cast, with low levels of star formation. There appears to be minimal dust obscuration, with a relatively smooth distribution of light across the system. The lack of apparent spiral arm structure or a well-defined disk suggests that any pre-existing disk structures have been disrupted or are in the process of being destroyed by the interaction.
