The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a somewhat elongated shape, tending towards an intermediate roundness rather than a perfectly circular or highly elongated form. While appearing largely undisturbed, subtle indications suggest minor internal disturbances or interactions. The galaxy does not display prominent spiral arms or a well-defined disk structure. The light distribution appears relatively uniform and diffuse, lacking any bright, distinct knots of star formation. Overall, the galaxy's morphology suggests a system undergoing, or having undergone, a period of quiescence with only minor ongoing dynamical activity.
