The galaxy appears to be a relatively smooth, spheroidal object. There is a central, bright bulge region that gradually fades into the surrounding galactic halo. The color profile suggests a higher concentration of older stellar populations towards the core, which emits a yellowish light. As you move away from the center, there are hints of bluer stellar populations, indicating possible regions of more recent, albeit subdued, star formation. The galaxy exhibits a slight ellipticity, appearing nearly round, but a closer inspection reveals a subtle deviation from perfect circularity. No obvious spiral arms or bar structures are apparent. There is no clear evidence of any significant tidal disturbances or ongoing major mergers. The overall morphology is indicative of an early-type galaxy that has largely exhausted its gas supply and is no longer experiencing vigorous star formation.
