The galaxy appears to be of intermediate type, exhibiting characteristics of both elliptical and spiral galaxies. The central region displays a smooth, concentrated morphology, possibly indicating an older stellar population. This region transitions into a less defined, more diffuse outer structure. There is evidence of a disk-like component. This is suggested by a slight flattening. The galaxy's overall form is largely spheroidal. As for color, the central region exhibits a yellow-red hue that shifts to blue-green in the outer regions. This suggests active star formation, but further data would be required to determine if the galaxy is undergoing any major disruptive events.
