The galaxy presents as a relatively smooth, centrally concentrated system. Its overall shape is elliptical, appearing mostly rounded with slight elongation. The galaxy exhibits a color gradient, with a yellowish-white hue dominating the core region, suggesting an older stellar population. The outer regions of the galaxy display a fainter and bluer color profile, potentially indicating the presence of some younger stars or ongoing, albeit low-level, star formation. There's no obvious presence of a prominent disk structure or spiral arms. No major or minor merging events are apparent. There may be some subtle distortions or minor disturbances in the outer regions, hinting at possible past interactions, but this is not definitively clear from the image.
