The galaxy appears to be a relatively smooth, elliptical or lenticular type. The central bulge is prominent and exhibits a bright, yellowish-white hue, suggesting a population of older stars. The overall shape is somewhat rounded, though not perfectly spherical, with a suggestion of a disk-like structure. There is a subtle color gradient from the core outwards, with the outer regions displaying a slightly redder color, possibly indicating dust or a shift in stellar population. There's a hint of some minor disturbance or asymmetry in the outer regions, but no clear indication of a major merger or significant tidal features. The structure appears relatively quiescent, with little evidence of active star formation across the disk.
