The galaxy presents a generally smooth, elliptical morphology. Its light profile is concentrated towards the center, exhibiting a bright core that gradually diffuses outwards. There are no distinct spiral arms or prominent features indicative of a disk structure. The overall shape is nearly round, though with some deviation from perfect circularity. Based on the color gradient visible, the central region appears to be dominated by older stellar populations, possibly exhibiting a lower rate of star formation. There is a slight suggestion of minor disturbance, which could be the result of gravitational interaction with another object.