The galaxy presents a somewhat elliptical morphology, exhibiting a smooth and centralized concentration of light. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central region. A gradual decrease in luminosity is observed moving from the core outwards, with no distinct spiral arms or prominent dust lanes visible. There appears to be a slight asymmetry in the outer regions, hinting at possible minor gravitational interactions or disturbances, though a clear merger event is not apparent in the image. The galaxy does not appear to be perfectly round. Considering its luminosity and estimated redshift, this galaxy likely represents a massive system. Star formation activity, if present, appears to be relatively low.
