The galaxy presents as a somewhat smooth, concentrated luminous object with a slight elongation. Its color profile indicates a population of stars that are likely older. There is a very subtle suggestion of a disk-like structure with a central bulge, but this is not well-defined. There appears to be a faint hint of possible interaction or minor disturbance with the even distribution of light near the galaxy. The overall morphology is generally consistent with an early-type galaxy such as an elliptical or lenticular galaxy. The object appears fairly isolated.
