The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. The light distribution is generally even, without prominent spiral arms or a distinct bar. The galaxy's color appears somewhat redder, suggesting an older stellar population. There is a subtle suggestion of a disk-like structure, but it is not a dominant feature. No signs of active galactic nuclei or ongoing major mergers are apparent. The galaxy's morphology is best described as an elliptical or lenticular galaxy.