The galaxy presents an overall elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. There is a concentration of light towards the central region, likely indicating a bulge component composed of older stellar populations. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/white, suggesting an older, passively evolving stellar population. The outer regions show a bluer hue, possibly indicating more recent star formation activity. The galaxy's shape is generally elliptical but appears slightly elongated. No major disturbances or signs of ongoing mergers are readily apparent, though a slight asymmetry in the light distribution warrants further investigation. The galaxy appears relatively isolated in the image field.
