The galaxy presents as an elongated structure with a significant degree of asymmetry. One end displays a bright, concentrated core region, exhibiting a yellowish-orange hue indicative of an older stellar population. Emanating from this core is a diffuse, bluish extension which seems to curve away. The blue color suggests ongoing star formation within this extended region. This extension is not uniform, showing irregularities and what appear to be clumpy structures indicative of tidal debris or interactions. The overall shape deviates significantly from a regular elliptical or spiral morphology, potentially suggesting an ongoing or recent merger event.
