The galaxy presents an elliptical morphology, although with some observable features suggesting the presence of a disk. The central region exhibits a high concentration of light, indicative of a substantial galactic bulge. The bulge appears relatively smooth in texture. The outer regions of the galaxy display a more diffuse and patchy structure, exhibiting some irregularity but maintaining a generally elliptical outline. There is a subtle hint of spiral arm structure, albeit not well-defined, suggesting a possible transition state or a galaxy with weak spiral arms. There seems to be some minor gravitational disturbance present in the galaxy, perhaps due to a minor merger, although the primary morphology is still mostly undisturbed. The galaxy's color suggests that it is not highly active in star formation.