This galaxy presents as a somewhat diffuse, elliptical-like structure. The central region exhibits a high degree of luminosity, appearing nearly spherical and smoothly distributed with a yellow/white hue, suggestive of an older stellar population dominating the core. Progressing outwards from this central bulge, the luminousity gradually diminishes, extending into a fainter, more amorphous halo. There is some subtle color variation within this region as the galaxy transitions from the central bulge into the outskirts of the galaxy, showing hints of blueish light. The isophotes are generally rounder than they are elongated. There may be some minor gravitational interaction occurring, as evidence by some visual irregularities in shape, but it is not a major merging event.
