The galaxy presents an elliptical morphology, with a notably smooth and concentrated central bulge. The light distribution appears relatively even, fading gradually from the bright core towards the edges. A slight elongation is discernible, suggesting it is not perfectly spherical. There is a faint, disk-like structure. No distinct spiral arms or significant dust lanes are observable within the galaxy, and the light emitted appears to originate from an older stellar population. The galaxy seems to be relatively isolated, with no clear signs of recent or ongoing major merger activity.