The galaxy presents a generally smooth, elliptical morphology. It appears elongated, with a high degree of axial ratio. The core of the galaxy exhibits a strong concentration of luminosity, indicative of a dense stellar population. Moving outward from the core, the luminosity gradually decreases, with no distinct spiral arm structures or prominent dust lanes visible. The color gradient suggests a potentially older stellar population dominating the galaxy, with a redder hue observed in the outer regions. There is a slight indication of minor disturbances in the outskirts, though the overall structure remains largely undisturbed.
