The galaxy appears to be a merging system. It displays significant morphological disturbance, characterized by an irregular shape and distorted features. The primary body is elongated, with an aspect ratio suggesting a deviation from sphericity towards a more cigar-like appearance. There is evidence of multiple distinct nuclei or concentrated regions of luminosity within the system, which could represent the cores of interacting galaxies. The overall color profile appears to be relatively red, with a hint of bluer components possibly indicating areas of active star formation. The presence of tidal tails or bridges of material extending outwards is not definitive but there may be some hint of a minor disturbance. The light is not uniform across the galaxy; it's brightest towards the center with the color profile becoming slightly more yellow.
