The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. Fainter, bluer extensions emanate from the central region, hinting at the presence of a younger, star-forming population. The overall shape is roughly circular. There is no clear evidence of a prominent disk structure, spiral arms, or major ongoing mergers. Faint signs of minor disturbances may be present, but the galaxy appears to be largely undisturbed.
