The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. Its overall shape tends towards roundness rather than a highly elongated or cigar-like form. There is a slight suggestion of a faint, extended disk component surrounding the central bulge, though it lacks well-defined spiral arms or prominent features. The color profile indicates a concentration of older stellar populations, particularly within the bulge, suggesting reduced levels of current star formation within this part of the galaxy. Hints of some minor disturbance in its structure may be present.
