The galaxy presents as a merging system with a disturbed morphology. A dominant, relatively smooth component, likely the core of one galaxy, displays a yellowish-orange hue suggesting an older stellar population. Connected to this central region is a smaller, more compact component, potentially another galactic core. There appears to be some color gradient within the system, with bluer tones visible at the edges indicating possible active star formation, although this is faint. The overall shape deviates significantly from a regular elliptical or spiral structure, exhibiting an irregular and elongated form, characteristic of gravitational interactions. The light profile suggests a high degree of central concentration.
