The galaxy presents as a somewhat irregular structure. It appears to be undergoing a significant interaction or merging event, showing no clear spiral or elliptical morphology. The light distribution suggests multiple nuclei or highly concentrated regions within the system, with a dominant central concentration surrounded by less distinct, extended features. Color variations suggest ongoing star formation in some regions, indicated by bluer tones, alongside older stellar populations with redder hues. Overall, the system exhibits a disturbed morphology indicative of a dynamic state. Tidal tails or bridges connecting the central mass to these surrounding features may be present.
