The galaxy presents as a predominantly smooth, elliptical structure. The light distribution is centrally concentrated with a gradual decline in brightness towards the outer regions. The core exhibits a yellowish hue, potentially indicating an older stellar population. There is minimal evidence of distinct spiral arms or dust lanes; however, the overall shape deviates slightly from perfectly spherical, exhibiting a weak elongation. There are no signs of major mergers but a hint of a minor disturbance. The red shift indicates that this is a galaxy at intermediate distance. Its size is moderate. It's star forming rate is low.
