The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated bulge. There is a subtle flattening of the galaxy along its major axis. The central region exhibits a yellowish hue, likely indicating an older stellar population. Moving outward from the core, the galaxy displays a faint, bluish disk component. The presence of this blue light suggests ongoing star formation within the outer regions. There is evidence of minor disturbances of disk, though no significant merging is present. The estimated size of the galaxy is approximately 7 kiloparsecs in radius.
