The galaxy appears to be relatively smooth and centrally concentrated, with a primarily elliptical morphology. There is little to no discernable disk structure or spiral arms. Its light distribution suggests a generally homogenous stellar population, with no particularly prominent star-forming regions visible. Faint asymmetries are noted and may indicate minor tidal disturbances. The color gradient transitions from blue to red, suggesting an older stellar population, and a suppression of star formation activity. It seems like the system may be undergoing minor interactions with neighboring galaxies, but no merger events are immediately apparent. The galaxy exhibits a rounded shape.
