The galaxy presents as a somewhat elliptical structure, with a smooth, unresolved appearance. The light distribution indicates a centrally concentrated luminosity profile, decreasing gradually towards the edges. There is no clear evidence of spiral arms, a central bar, or any distinct features typically associated with disk galaxies. The galaxy does not appear perfectly spherical, displaying a subtle elongation. There might be a slight indication of minor disturbance in the galaxy, but it does not seem to be undergoing a major merging event. 
