This galaxy presents as a relatively smooth, centralized structure with an elliptical morphology. The central region exhibits a yellowish-orange hue, suggesting a population of older stars. There is a subtle color gradient transitioning from the core outward, with the outer regions displaying slightly redder tones, potentially indicating a decrease in younger stellar populations. The lack of distinct spiral arms or prominent dust lanes indicates a classification towards early-type galaxies. There is a hint of asymmetrical structure but that is most likely due to image quality. The overall appearance suggests a galaxy that is not currently undergoing significant star formation, and may be nearing the end of its active period. The galaxy appears to be relatively isolated, showing no immediate signs of ongoing major mergers or tidal disturbances.
