The galaxy appears to be largely smooth in structure, presenting a centrally concentrated luminosity profile. It exhibits a somewhat elliptical morphology, with a shape that is tending towards round. There is evidence of a possible minor disturbance in the disk, suggesting it may be interacting with another galaxy or experiencing internal disruptions. The central region is bright and distinct, indicating a significant concentration of stars. There is a faint blueish region extending from the central region, potentially indicating active star formation in this region.
