The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a diffuse, elliptical morphology, with a brighter core region. There is a slight asymmetry in the galaxy's light distribution, with a subtle extension or disturbance visible on one side. The color profile suggests a mixture of stellar populations, with bluer hues concentrated towards the central region and redder tones in the outer parts. Overall, the galaxy does not show strong evidence of spiral arms or a well-defined disk structure.
