The galaxy presents a generally elliptical morphology, appearing elongated with a moderately high ellipticity. A central bulge region is prominent, exhibiting a bright, concentrated luminosity. The color profile transitions from a yellowish-white core to fainter, redder outskirts. There is a discernible decrease in surface brightness as one moves from the central region outward. The smoothness of the galaxy suggests a relatively evolved system, with no obvious signs of strong spiral arm structures or active star-forming regions visible in this optical band. Subtle color variations may indicate variations in stellar populations or dust content within the galaxy. There is no clear evidence of tidal disturbances or ongoing merger events.
