The galaxy appears as a centrally concentrated object with a slightly elongated morphology. The core exhibits a bright, relatively uniform color, suggesting an older stellar population. Moving outward from the center, a fainter, bluer halo becomes apparent, likely indicative of ongoing or recent star formation activity. The overall structure is dominated by a smooth, diffuse light profile with only subtle indications of spiral arm features or distinct substructures. The morphology leans towards an elliptical or lenticular classification, showing characteristics of both, but the slight disk-like structure pushes it away from being purely elliptical. There seems to be some minor asymmetry, potentially caused by recent interactions or internal processes. This galaxy is likely a massive system with moderate levels of current star formation.
