The galaxy presents a generally smooth, elliptical morphology. Its central region displays a concentrated, yellowish-white luminosity, suggesting an older stellar population. Fainter, bluish-white light extends outwards from the core, indicating the presence of a younger, bluer stellar population. The galaxy exhibits no prominent spiral arms or bar structures, appearing relatively undisturbed. A subtle asymmetry is present, with a slight elongation. Overall, the galaxy appears to be a relatively massive system with a modest rate of star formation.
