This galaxy presents as a generally smooth and rounded structure, appearing more elliptical than spiral in form. It exhibits a concentrated central bulge, which appears a yellowish hue, possibly indicating an older stellar population. The galaxy extends outwards with a gradual decrease in intensity, suggesting a decreasing stellar density towards its periphery. There is a slight hint of disk-like structure with a very faint blue hue, suggesting some recent star formation. Overall, this galaxy seems to be a relatively massive system at a considerable distance, with an overall shape that is generally undisturbed, but with a few features suggesting some past interactions.
