This galaxy presents an elliptical morphology. The central region exhibits a concentrated, bright luminosity with a yellowish hue, suggesting an older stellar population. Moving outward from the core, the light gradually diffuses into a bluish halo, possibly indicating a younger stellar population or ongoing star formation within the galactic disk. There are no apparent spiral arms or a prominent dust lane. The overall smoothness of the galaxy indicates that it is likely a mature system, potentially with a relatively low current star formation rate. There is a slight elongation of the object along a major axis that can be observed, moving it away from being spherical. No nearby merger events are visible.
