The galaxy presents an overall smooth morphology, appearing elliptical in shape with a high degree of roundness. The galaxy's core exhibits a bright, concentrated luminosity, suggesting a significant stellar density in the central region. Color gradients within the galaxy indicate a possible variation in stellar populations, with the core displaying a yellower hue indicative of older stars, transitioning to somewhat bluer tones in the outer regions. This could suggest recent or ongoing, though subdued, star formation in the outer parts of the galaxy. Evidences suggest that this galaxy may be undergoing or have experienced a minor interaction with another galaxy.
