The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical profile with no discernible spiral arms or disk-like structure. The light distribution is concentrated towards the center, suggesting a prominent galactic nucleus or bulge. The color gradient indicates a dominant population of older stars, with a yellowish hue suggesting relatively low ongoing star formation activity. There is no evidence of significant dust lanes or recent merger events. The overall morphology suggests an evolved system that has largely exhausted its gas reservoir. The galaxy appears well-defined and isolated, showing no obvious signs of interaction with nearby galaxies.
