The galaxy appears to exhibit a morphology that is neither completely smooth nor a well-defined spiral or elliptical structure. There appears to be a central bulge region, but the overall form is somewhat irregular and disturbed. There's evidence of possible tidal interactions, with some disrupted features extending outwards. There are some features of what looks like disks, but they seem to be disrupted. Color gradients are present, with bluer hues in some regions, potentially indicating areas of recent star formation, and redder hues elsewhere, which may be areas of older stellar populations. The object shows possible signs of an ongoing or recent merger event.
