The galaxy presents as an elliptical structure with a noticeable bulge, elongated along a discernible major axis. The central region exhibits a bright, concentrated luminosity, indicative of a dense stellar population. A color gradient is apparent, transitioning from a yellowish-white hue at the core to a bluer tint towards the outer edges. This color variation suggests the presence of younger, hotter stars in the galaxy's periphery, while the core is dominated by older, cooler stars. There appears to be a disk structure present in the outer regions of the galaxy. The galaxy does not show strong evidence of spiral arms. The overall appearance is relatively smooth, lacking pronounced features that would indicate significant ongoing star formation. The ellipticity of the galaxy is moderate, and the surface brightness fades gradually from the center outwards, suggesting a relatively diffuse halo. There does not appear to be any signs of recent or ongoing mergers.
