The galaxy presents a relatively smooth morphology, exhibiting a predominantly rounded shape. There is a suggestion of a slight disk-like structure, though the overall appearance is more akin to an elliptical galaxy. No clear spiral arms or bar features are discernible. The galaxy appears to be undergoing minimal, if any, significant merging activity or major disturbances. There is the possibility of a very minor disturbance visible on the lower corner of the galaxy, though this could also be an artifact of the image. The color profile indicates the presence of an older stellar population, though there may be the presence of an older disk that is bluer in color. The light is centrally concentrated, with a gradual decline in surface brightness towards the outer regions.
