The galaxy presents a primarily smooth and luminous appearance. The central region exhibits a concentrated, bright yellowish-orange hue, indicative of an older stellar population. Surrounding the core is a fainter, more diffuse halo of light extending outwards, with a slight elongation suggesting an elliptical shape. There is a faint blue tinge on the left side of the galaxy, which could suggest a small amount of star formation is occuring. No distinct spiral arms or dust lanes are readily apparent. The galaxy appears relatively isolated, showing little evidence of major tidal disturbances or ongoing merger activity. Overall, it appears to be a massive galaxy with a red shift of around 0.25.