The galaxy presents a generally smooth morphology, appearing largely elliptical in shape but not perfectly rounded. There's a suggestion of a slight elongation. The central region is noticeably brighter and exhibits a yellow-orange hue, implying an older stellar population dominating the core. This core region smoothly transitions outward to a fainter, bluer halo or disk component. The blue color suggests the presence of younger stars and possibly ongoing star formation, although the smoothness of the structure indicates it is not vigorous. There is a hint of minor disturbance in the outer regions, although this is difficult to ascertain at this resolution. The galaxy appears relatively isolated, with no obvious signs of a major merger event. Overall, the galaxy gives the impression of a mature system with a mix of stellar populations, experiencing a low level of ongoing star formation.
