The galaxy presents a relatively smooth morphology with no distinct spiral arm structures visible. It appears roughly elliptical, though not perfectly circular. The color profile indicates a dominance of older stellar populations, exhibiting a reddish-yellow hue. There is little evidence of ongoing major star formation; it seems to be a more quiescent system. No significant tidal disturbances or indications of recent major mergers are readily apparent. A slight asymmetry can be observed in the galaxy's overall shape, hinting at the possibility of a minor interaction or past merger event that has largely settled.
