The galaxy appears as an elliptical-type object. The central bulge exhibits a smooth, concentrated luminosity profile, appearing mostly red and indicative of an older stellar population. Fainter, greenish hues extend outward, suggesting the presence of some younger stars and possibly ongoing, but limited, star formation within the disk component. The overall morphology displays a somewhat rounded appearance with an intermediate shape between circular and elongated. There is a subtle suggestion of minor disturbance in the galaxy's structure, but no clear signs of a major merger are apparent. The relative colors indicate a moderate mass system with ongoing star formation, although the bulge exhibits an older stellar population.
