The galaxy presents as a centrally concentrated spheroid with a smooth morphology. The core exhibits a yellowish-white hue, indicative of an older stellar population and minimal ongoing star formation within that region. Surrounding the core, a fainter, bluish halo is observed, suggesting the presence of a younger stellar population, or potentially scattered light. No distinct spiral arms or disk-like structures are discernible, suggesting the galaxy is an elliptical type. There are no obvious signs of recent major mergers or tidal disturbances, with an overall regular shape. The galaxy is relatively compact.
