The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The central region exhibits a high surface brightness, suggesting a concentrated nucleus. There's a noticeable elongation along a particular axis, indicating a moderate degree of ellipticity. The color gradient transitions from a yellowish hue in the central bulge to a slightly bluer shade in the outer regions, hinting at a variance in stellar populations across the galaxy. Subtle distortions or irregularities are observed in the outer regions, which might suggest minor gravitational interactions or recent accretion events. Overall, the galaxy appears to be a massive system with moderate ongoing star formation activity.
