The galaxy presents as an elliptical morphology with a relatively smooth appearance. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population and potentially an active galactic nucleus. Moving outward from the center, the light intensity decreases gradually, indicating a radial decline in stellar density. The overall color of the galaxy is slightly yellow, possibly indicative of an older stellar population. There are some slight disturbances and color changes, but not significant enough to suggest recent merger activity. There appears to be a close companion that shows signs of star formation, as well as another possible galaxy behind the primary, though its distance is uncertain.
