The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It appears relatively smooth in texture with a concentrated central bulge, exhibiting a fairly even light distribution across its body. There's a slight elongation present, and a hint of a disk structure might be present. The galaxy is a redder hue, suggesting a population of older stars and a relatively low star formation rate. There isn't much evidence of ongoing mergers or major disturbances. It is reasonably large and massive.
