The galaxy presents a generally smooth morphology, with a notable absence of distinct spiral arm structures or a prominent central bar. The light distribution suggests a dominant spheroid component. It appears to be an elliptical galaxy, or perhaps a lenticular galaxy seen face-on. There may be a disk component. The color gradient indicates an aging stellar population. The central region shows an increased concentration of yellow light, likely associated with older, redder stars. Fainter, bluer emission is present in the surrounding regions, suggesting possible ongoing, albeit low, star formation. The galaxy is slightly elongated. There is no obvious major merger event occurring, but there might be some tidal disturbances.