The galaxy presents as an elliptical morphology, with a high degree of central concentration. The core region is luminous and exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the luminosity decreases, and the color shifts subtly towards a redder tone. The outer regions of the galaxy appear smooth and featureless, with no discernable spiral arms or significant dust lanes. There is no evidence of ongoing major mergers or significant tidal disturbances. The galaxy is approximately round, with very little ellipticity observed. Overall, the galaxy appears to be a passively evolving system, with little current star formation activity.
