The galaxy appears to be a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The light distribution suggests a dominant bulge component. There is a hint of a disk. The color profile of the galaxy indicates a redder core transitioning to slightly bluer hues in the outer regions. This color gradient could be indicative of differing stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars in the disk. There is no strong evidence of ongoing major merging activity. The overall structure suggests a galaxy that has largely completed its formation.
