The galaxy appears as a centrally concentrated object, exhibiting a smooth morphology. Its shape is largely elliptical, tending toward somewhat of an intermediate, but still elliptical, form. There are no readily apparent spiral arms or a prominent disk structure.

The galaxy's color profile appears to be generally uniform, with a slight concentration of yellow light toward the center and a reduction of yellow light towards the fringes. This color suggests a relatively older stellar population dominating the galaxy's composition, with minimal ongoing star formation. There are no major signs of tidal disturbances or ongoing mergers, with only minor disturbances possibly present. The high degree of smoothness, coupled with the apparent elliptical shape and color profile, suggests that this is a relatively evolved galaxy.
