The galaxy presents an elliptical morphology, exhibiting a somewhat diffuse structure without prominent spiral arms or a distinct central bulge. The color distribution appears to be relatively uniform across the galaxy, with a slight blue tint, suggesting the presence of some younger stellar populations, although the overall color indicates that the galaxy is composed mostly of older stars. There are subtle signs of disturbance within the galaxy's light distribution, possibly resulting from minor gravitational interactions or recent mergers. The object's moderate ellipticity indicates that it may not be a perfectly spherical system, with the general axis rotated significantly from the vertical.
