The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, centrally concentrated light distribution. It shows a high degree of central concentration, indicated by the bright, yellowish core that gradually fades into the outer regions. There is a slight elongation to its overall shape, suggesting it is not perfectly spherical but instead more spheroidal. While there is some variation in color across the galaxy, it appears relatively uniform, lacking prominent distinct features such as spiral arms or significant dust lanes. The color gradients suggest that the central regions are composed of older stellar populations with a decrease in age towards the outer regions. No apparent signs of ongoing major mergers or significant tidal disturbances are visible.
