The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated brightness, appearing nearly spherical. A slight elongation is visible, hinting at a possible disk-like component, though this is not immediately obvious. The color appears largely homogenous, with a predominantly reddish hue. The galaxy is not completely isolated, as there appears to be another galaxy in the process of merging with it, as there is visible disturbance to its overall circular shape. The mass is quite high and the star formation rate is quite low.