This galaxy appears to be a relatively smooth, elliptical or lenticular system. Its overall form is largely spheroidal, with no strong evidence of spiral arm structures or a prominent galactic disk. A smooth gradient in luminosity is apparent, with a bright, concentrated core region exhibiting a redder color index, possibly indicating an older stellar population or higher dust extinction. The outer regions are fainter with slightly bluer colors. There is no obvious tidal distortion or interaction with neighboring galaxies. Given the overall morphology, this galaxy is likely a high mass system with relatively low ongoing star formation.
