The galaxy presents as a moderately luminous object with a generally smooth, elliptical morphology. There is little evidence of spiral arm structure or a prominent disk. The light distribution suggests a concentration of stars toward the center, which is typical for this morphology. The galaxy exhibits a color gradient, appearing more yellow towards the center and slightly bluer in the outer regions. This color variation could indicate differing stellar populations within the galaxy, where the center hosts older, redder stars, while the outskirts contain younger, bluer stars. However, this color variation could also be the result of differential dust extinction within the galaxy, where more dust obscures blue light from the central regions. There may be some minor asymmetries within the galaxy that would indicate it is experiencing, or has experienced some sort of gravitational disturbance.
