The galaxy appears to be undergoing a major merger event. The morphology suggests two distinct nuclei or high density regions within a common, distorted halo of light. Tidal tails are visible extending from the main body, indicative of gravitational interaction. The overall color profile leans towards a redder hue, which could imply an older stellar population and/or significant dust obscuration, yet there also appears to be light indicative of a younger population of stars. The central regions of the galaxy exhibit more concentrated light, possibly associated with the galactic nuclei. The shape deviates significantly from a simple elliptical or spiral form, with an elongated and irregular structure caused by the ongoing merger process.
