The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of central concentration. The light distribution exhibits a noticeable radial gradient, with the core region being significantly brighter than the surrounding halo. The overall color profile is redder, suggesting an older stellar population and a reduced rate of ongoing star formation. There is no visible evidence of spiral arms, a bar structure, or significant dust lanes. Subtle asymmetries could indicate minor gravitational interactions, but no major disturbances or merger events are apparent in this image. The galaxy’s shape is generally elliptical but appears slightly elongated.
