The galaxy presents as a system undergoing significant interaction or disturbance. The morphology suggests a possible merger event or strong tidal interaction with a nearby galaxy, evidenced by asymmetry and irregular features. The central region appears relatively smooth and concentrated, exhibiting a yellowish hue, which may indicate an older stellar population dominating the core. Fainter, bluer regions are observed surrounding the core, perhaps indicating ongoing star formation. There is one other distinct area of concentrated light relatively close to the main body of the galaxy, which may be an area of high star formation, or another remnant of a past merger event. The overall shape deviates significantly from a regular elliptical or spiral form, with distortions present in the outer regions.
