The galaxy appears to be a relatively smooth, elliptical structure with a high degree of central concentration. There is a bright, yellowish core, potentially indicative of an older stellar population or an active galactic nucleus. The outer regions of the galaxy display a gradual decrease in luminosity and a bluer hue, which may imply the presence of a younger stellar population or ongoing star formation, although limited. The overall morphology suggests a galaxy that is primarily spheroid in shape, with a suggestion of elongation. No distinct spiral arms or prominent dust lanes are visible. There is some indication of a minor disturbance in its overall shape.
