The galaxy presents an elliptical morphology, appearing somewhat elongated or cigar-shaped in its overall form. Its light is dominated by yellowish-orange hues, concentrated towards the central region of the galaxy, suggesting an older stellar population in the bulge. Fainter bluish-green hues are present along the galactic disc or outer regions, implying the possibility of some ongoing star formation, though it appears quite subdued. The galaxy's structure seems largely smooth, exhibiting a high degree of central concentration with a gradual decrease in luminosity toward its outer edges. There are no obvious signs of tidal tails, strong asymmetries, or significant disturbances. It is likely a massive galaxy with a significant population of evolved stars.
