The galaxy exhibits a smooth morphology with a central bulge that appears nearly spheroidal. The primary light source originates in the core of the galaxy with an apparent yellow to white glow. This light then disperses into an oval shape extending outward from the central core, which is then surrounded by a darker galactic halo. The color profile of the outer disk is slightly redder than the central bulge. The structure is not perfectly circular, exhibiting a slight elongation. There is no clear evidence of spiral arms or significant dust lanes. There are no signs of merging or major disturbances. The galaxy appears to be a relatively isolated system in a mature stage of evolution.
