The galaxy presents as a system with potential ongoing or past merger activity. The primary component exhibits a somewhat elliptical morphology, with a brighter, more concentrated central region. There is evidence of disturbed structure, possibly tidal features or distorted arms, particularly in the form of a fainter, elongated extension emanating from the main body, giving it an irregular shape. The color distribution suggests a mix of stellar populations, with a bluer hue in some regions, potentially indicating areas of more recent star formation, and redder hues indicating a population of older stars. There are potentially three or more individual components, with one appearing to be in close proximity and in the process of interacting or merging with the primary component.
