The galaxy presents as a largely smooth and centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of roundness. The central region displays a brighter, more intense luminosity, gradually fading into the outer regions. There is a subtle color gradient from the core outwards, becoming redder as it moves outward. No obvious spiral arm structures or significant dust lanes are discernible within the galaxy's morphology. There appears to be no prominent ongoing major merger events affecting the galaxy's overall structure, but a very minor disturbance could be possible. The overall light distribution indicates a system dominated by an older stellar population, with a low rate of star formation. The size of the galaxy appears moderately extended, but not exceptionally large.
