The galaxy presents a largely smooth morphology, appearing as a concentrated central bulge with a gradual decrease in luminosity extending outwards. The color profile suggests a dominant population of older stars, as evidenced by the yellowish-red hue, implying low current star formation activity. The galaxy exhibits an elliptical shape with a high degree of central concentration. Evident in the galaxy is that it shows no signs of spiral arms or a distinct disk structure. There are no obvious signs of tidal interactions or recent merger events, as the galaxy appears undisturbed. Overall, this galaxy appears to be an evolved, early-type galaxy with little ongoing star formation.
