The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction with another galactic body. A faint tidal tail or bridge appears to connect the two brightest regions, suggesting gravitational interaction. The color profile of the galaxy appears to be complex, with regions of bluer light interspersed with redder components. This indicates varied stellar populations and potentially ongoing star formation. The galaxy is neither perfectly elliptical nor a well-defined spiral, falling instead somewhere in between, indicating a transition state. The bright, centralized light suggests a significant bulge component.
