The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. It exhibits a yellowish hue, suggestive of an older stellar population. There is a slight elongation in its morphology, but it is generally rounded in shape. No distinct spiral arms or prominent dust lanes are visible. There are some subtle variations in color and luminosity within the galaxy's halo, but overall, it appears undisturbed and relatively isolated. There are no indications of major mergers or significant tidal interactions. Based on the apparent color gradients, star formation rates are likely low.
