The galaxy appears as a nearly circular, well-defined spheroid. The central region exhibits a concentrated, bright, yellowish-orange glow, suggesting a significant population of older stars. Moving outwards from the core, the light gradually fades into a more diffuse halo. The color shifts subtly to include hints of redder tones in the outer regions. There are no readily discernible spiral arms or prominent dust lanes visible in this image. The overall impression is that of an elliptical galaxy with a smooth, relatively homogenous structure. There is no clear evidence of ongoing major mergers or tidal disturbances, although some slight asymmetry in the outer halo might suggest minor interactions in the past.
