The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. The core region displays a yellow-orange hue, potentially indicating an older stellar population and/or dust obscuration. A fainter, more diffuse halo surrounds the core, with hints of blue-ish and green-ish light, suggesting the presence of a younger stellar population and regions of ongoing star formation, albeit at a low rate. There is a small secondary bright region that appears to be separate from the central portion of the galaxy. The overall shape approximates a slightly elongated sphere, with no clear evidence of spiral arms or a well-defined disk structure. The morphology suggests that the object might be an elliptical galaxy. Evidences suggest that there is a possible merging event occuring.
