This galaxy presents a disturbed morphology, exhibiting features suggestive of an ongoing or recent merger event. The central region displays a bright, concentrated luminosity, possibly indicating a highly active galactic nucleus or intense star formation activity. Extending outwards from the core, there appears to be diffuse stellar material, possibly remnants of tidal tails or disrupted spiral arms. The overall shape is elongated and irregular, deviating significantly from a typical elliptical or spiral structure. The color gradient shifts from a yellow-orange hue near the center to a bluer tint in the outer regions, possibly implying a difference in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars more prevalent in the outskirts. Patches of lighter color could denote areas of heightened star formation. There is no clearly defined disk structure, lending credence to the classification as an irregular galaxy experiencing strong gravitational interactions.
