The galaxy presents as a relatively smooth and rounded structure. Its overall color appears to be yellowish-orange, suggesting a dominant population of older stars. No distinct spiral arms or a prominent disk structure are readily apparent. There is a slight concentration of luminosity toward the center, indicative of a galactic nucleus or bulge. No major disturbances such as tidal tails or obvious signs of a recent merger event are observed. The galaxy appears relatively isolated in this field of view.
