The galaxy presents as an elliptical morphology, appearing generally smooth with no distinct spiral arm structures or a central bar visible. There is a concentration of light towards the center, suggesting a bright galactic nucleus. The light distribution gradually diminishes outward from the core. The overall color is a yellowish-white hue, indicative of an older stellar population and suggesting ongoing star formation. The galaxy is slightly elongated. There is no evidence of major mergers or significant tidal disturbances in this image, although there are hints of minor disturbances.
