The galaxy presents an elliptical morphology, appearing somewhat cigar-shaped with a higher concentration of light in its central region. A smooth luminosity gradient is observed from the core outwards, with a gradual decrease in surface brightness towards the edges. The galaxy exhibits a dominant yellowish-orange hue, especially prominent in the central bulge, suggesting an older stellar population. Fainter, diffuse bluish regions are subtly interspersed around the main body, possibly indicative of some level of recent or ongoing star formation. No distinct spiral arms or well-defined disk structure are apparent. There are some slight disturbances in the galactic halo, hinting at potential minor interaction or past merger events. The overall structure appears relatively undisturbed, suggesting that the galaxy is not undergoing any major merger activity at the present time.
