The galaxy appears as a slightly elongated, diffuse object. It exhibits a central concentration of light that fades gradually outwards. The core region presents a yellowish hue, potentially indicating an older stellar population. Surrounding the core, a bluer, more extended envelope is visible, suggestive of ongoing star formation. There are no distinct spiral arms or a pronounced disk structure observed in the image. The overall morphology is relatively smooth, with minor irregularities that could indicate some disturbances or interactions but do not point toward a major ongoing merger. The shape leans towards being somewhere between perfectly round and elongated.
