The galaxy appears as a somewhat elongated, elliptical structure. It exhibits a centrally concentrated brightness profile, suggesting a bulge-dominated morphology. The core region presents a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the galactic disk fades into a bluish color gradient, which could be attributed to the presence of younger, bluer stars and possibly ongoing star formation within the outer regions, however at a low rate. There is a subtle indication of a faint and diffuse outer halo surrounding the main body. No distinct spiral arm structures are visible; overall the galaxy presents a smooth, relatively undisturbed appearance, with no clear signs of major mergers or tidal disturbances.
