The galaxy appears to be a relatively smooth, elliptical-type system. The core exhibits a concentrated, bright luminosity, indicative of a high stellar density or potential active galactic nucleus. The isophotes are generally elliptical with a slight elongation, and the overall shape is moderately round. There are no obvious signs of prominent spiral arms or significant dust lanes. The color gradient suggests an aging stellar population, appearing reddish-gold toward the core, which likely indicates a dominance of older, redder stars. There's minimal evidence of recent or ongoing major mergers, though the hint of asymmetry could imply a previous minor interaction. Overall, the galaxy presents as a mature system with a relatively quiescent star formation rate.
