The galaxy presents as a relatively smooth, centrally concentrated elliptical. It exhibits a rounded morphology with an apparent lack of significant disk-like features or spiral arms. The central region displays a bright, yellowish hue, suggesting a population of older stars. A gradual decrease in surface brightness is observed moving outward from the core, with a diffuse, fainter halo extending beyond the brighter central region. There is no obvious indication of recent major merging activity or strong tidal disturbances. Faint blue regions may be present in the outer edges of the halo, which may indicate regions of possible star formation.
