The galaxy presents as a somewhat elliptical, moderately luminous object with a discernible, though not sharply defined, central bulge. The overall color profile suggests an older stellar population, with a yellowish hue dominating the central region. There's a subtle gradient in color extending outward from the core, transitioning to a slightly bluer tint in the surrounding halo, which may indicate regions of more recent, though subdued, star formation. No spiral arm structure is readily apparent. Some minor disturbances seem to affect the symmetry of the galaxy. There is a hint of possible interaction, or perhaps a minor disturbance within the galactic structure. The galaxy does not display strong indications of a major ongoing merger event. The galaxy appears to be neither perfectly round nor highly elongated.
