This galaxy appears to be a relatively smooth, elliptical or lenticular type. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. The light appears to diminish gradually from the center outwards, indicating no prominent spiral arm structures. There's a hint of bluer light further from the center, suggestive of some younger stars, though the galaxy is primarily dominated by older stars. There are no prominent dust lanes or signs of ongoing, major star formation activity. Overall, the galaxy displays a symmetrical and well-defined structure with a moderate degree of roundness. It shows no visual indicators of significant tidal disturbances or interaction with other galaxies.
