The galaxy presents as an elliptical morphology. It exhibits a smooth, concentrated light profile with no discernible spiral arm structure. The shape is moderately elongated. There is a lack of significant dust lanes or prominent star-forming regions. The galaxy appears to be relatively isolated, with no indications of major tidal disturbances or ongoing merger events. The central region displays a brighter concentration of light, suggesting a possible galactic nucleus. Overall, the galaxy appears to be a relatively evolved system with minimal ongoing star formation.
