This galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge, which dominates the overall light profile. The color of the bulge appears slightly redder than the outer regions, suggesting an older stellar population. The surrounding disk, if present, is faint and lacks distinct spiral arm structure, appearing more like a diffuse halo. There may be minor disturbances in the outer regions, but overall, the galaxy doesn't show strong evidence of a major merger event.
