The galaxy presents a predominantly smooth morphology with a concentrated central bulge that graduates into a more diffuse halo. The overall shape appears to be roughly elliptical with a slight deviation from perfect circularity. The light distribution suggests a relatively even population of stars throughout the galaxy, although some minor irregularities may be present in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. The color profile indicates a bias toward older stellar populations, indicated by a redder central region transitioning to a bluer halo region. There is a possibility of a recent minor disturbance or a past merger event, though the galaxy does not show major signs of interaction with another galaxy.
