The galaxy exhibits a generally smooth morphology, appearing largely elliptical or lenticular in shape. The central bulge is prominent and displays a concentrated, bright yellowish hue, suggesting an older stellar population. The outer regions show a fainter, more diffuse structure with a bluer color component, hinting at the presence of some younger stars or ongoing, but very limited, star formation within the galaxy's disk. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively isolated, showing no obvious signs of interaction with nearby galaxies. The overall color gradient suggests a declining star formation rate from the outer edges towards the core.
