The galaxy presents an overall elliptical morphology, appearing relatively smooth and concentrated towards the center. Its major axis is discernibly larger than its minor axis, resulting in a somewhat elongated, cigar-shaped appearance. The central region exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the light gradually fades, displaying a smoother distribution, though subtle variations are visible. There's a hint of bluer light within the galaxy, indicative of ongoing, albeit limited, star formation. No strong spiral arm structures or obvious signs of major merger events are apparent from visual inspection. The galaxy appears generally undisturbed with only slight irregularities.
