The galaxy presents a smooth, elliptical morphology, exhibiting a notable central bulge. The light distribution appears relatively uniform, lacking distinct spiral arm structures. A slight flattening is visible, deviating from a perfectly circular shape. There is a subtle color gradient, transitioning from a warmer, yellowish core to cooler, bluish outer regions. This may indicate differential stellar populations with older stars in the bulge and younger stars in the surrounding disk. There is no apparent dust lane obscuring the central region, nor any sign of active galactic nuclei activity based on visible light. The lack of any significant morphological disturbances suggests it is not currently undergoing a major merger. There might be a minor gravitational interaction occurring, given the slight warping of its disk shape. 
