The galaxy presents as a largely elliptical object with a smooth, diffuse light distribution. Its central region appears significantly brighter and more concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Extending outwards from the core is a fainter, more extended halo, also with a yellowish-white color. A localized reddish region is present within the halo, possibly indicative of a region of active star formation or dust obscuration. The galaxy does not show any prominent spiral arms or other distinct features typically associated with disk galaxies. There is minimal evidence of recent merger activity or significant morphological disturbance. The galaxy is reasonably compact, but not entirely spheroidal, appearing slightly elongated along one axis.
