The galaxy presents as a concentrated, elliptical form, appearing largely smooth in structure. The light distribution is dominated by a central bulge, with a radial decrease in surface brightness. The core displays a yellow-orange hue, potentially indicating an older stellar population with a lower rate of current star formation. The lack of prominent spiral arms or dust lanes suggests that this galaxy is a relatively evolved system. It is also notable for its compactness. There are no nearby objects to suggest it may be merging.
