The galaxy appears to be a merging system or a galaxy with a significant tidal disturbance. There are two distinct luminous components visible. The primary, larger component has a yellowish-orange hue suggesting an older stellar population. This component exhibits a somewhat elliptical morphology, appearing relatively smooth with only a subtle deviation from perfect radial symmetry, potentially indicating a minor interaction. A secondary, smaller component to the upper left of the primary component is visible, appearing as a fainter and bluer region, implying a younger stellar population or active star formation. The separation between the components suggests a possible late-stage merger or a galaxy with a close companion experiencing significant tidal effects. There are no obvious spiral arm structures or a prominent central bulge visible within the resolution limitations. The system appears to be generally compact.
