The galaxy presents as a system with evidence of ongoing or recent interaction. Its general morphology appears smooth, with a somewhat disturbed structure. The primary component is a central, roundish bulge. There are distinct regions of concentrated light, possibly indicative of multiple merging galaxies or distinct galactic nuclei within a single, larger structure. These brighter regions are embedded in a more diffuse halo of light, giving the galaxy a hazy appearance. Some areas exhibit a yellow-white color, suggesting a population of older stars. Given the disturbed morphology, the galaxy system likely has a complex mass distribution and star formation history.
