The galaxy presents a predominantly smooth morphology. The central region exhibits a pronounced concentration of light, appearing nearly spherical. The overall shape is somewhere between round and elliptical, showing a slight elongation. There is no immediately obvious spiral structure or prominent disk. Subtle color gradients are present, with the central bulge tending towards yellow and the outer regions appearing slightly more reddish. There are no distinct tidal tails or other obvious signs of a major ongoing merger, though there could be minor disturbances present. There appears to be a nearby object that could be a smaller galaxy that may be causing said disturbances. The galaxy likely has a high stellar mass. Star formation may be relatively low, with a high likelihood of mostly older stars.
