The galaxy appears to be relatively smooth in overall structure. There's a hint of elongation, suggesting it may not be perfectly spherical. The color profile indicates a central concentration of older stars, emitting light in the redder part of the spectrum. Fainter, bluer regions are discernible towards the outer edges, possibly indicative of some on-going star formation, although at a low rate. There's no strong evidence of a spiral structure, or a prominent, well-defined disk. No major mergers or strong tidal disturbances appear to be apparent.
