The galaxy presents as a relatively smooth and centralized object. Its morphology appears mostly elliptical, though the disk is hard to discern. There is a slight elongation and a subtle fading towards the edges. The light profile suggests a high degree of central concentration. Faint blue coloring is mostly uniform throughout, indicating the likely presence of young, hot stars. The galaxy does not exhibit any obvious signs of major disturbances from external interactions. The structure doesn't showcase any features that immediately suggest recent mergers or tidal tails. Based on the relative uniformity and lack of defined spiral arms, it might be evolving into a more spheroidal form. Overall, the galaxy's appearance indicates it is likely an elliptical or lenticular galaxy with a moderate amount of recent or ongoing star formation.
