This galaxy presents as a relatively compact object. It exhibits a somewhat irregular morphology, not conforming strictly to a spiral or elliptical classification. The color distribution suggests active star formation regions, indicated by the concentration of blue hues in the more visibly defined areas. There is a central concentration of light, potentially suggesting a bulge or a central supermassive black hole. Evidence of possible tidal disturbances and or minor mergers are weakly visible, but appear to be a very small disturbances and do not significantly disrupt the overall structure. There is no discernible spiral arm structure or bar feature.
