The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical type, lacking prominent spiral arms or a well-defined disk structure. The central region exhibits a brighter, more condensed concentration of light, likely representing the galactic nucleus. Moving outwards from the center, the light gradually diminishes, forming a somewhat diffuse halo. There's a slight elongation in its overall shape, though it appears mostly rounded. The color profile indicates a prevalence of older stellar populations, with a yellowish-red hue dominating the overall light emission. The rate of star formation is likely low. Based on its appearance, this galaxy seems to be a relatively isolated system, showing no immediate signs of major mergers or significant tidal disturbances. However, some minor asymmetries or disturbances cannot be ruled out, given the limited resolution.
