The galaxy presents as a centrally concentrated system, exhibiting a predominantly smooth, spheroidal morphology. The core region displays a yellowish hue, suggestive of an older stellar population. Surrounding the core, a fainter, bluish halo is observed, indicating the presence of younger, star-forming regions. The overall shape appears approximately round. There are no obvious signs of major tidal disturbances or ongoing merger activity. The light distribution is relatively even, with no distinct spiral arms or prominent dust lanes visible.
