The galaxy presents as a relatively smooth, elliptical morphology. The light profile suggests a central bulge that dominates the overall luminosity and is significantly brighter than the surrounding regions. This bulge appears nearly spherical. Moving outward from the core, there's a diffuse halo or extended envelope with a bluer color, suggesting a population of younger stars compared to the bulge. There is no strong indication of spiral arms or distinct features typically associated with disk galaxies; therefore the galaxy may be elliptical or lenticular. There is no indication of major disturbances, like merging activity. The galaxy is neither perfectly round nor highly elongated, showing an intermediate shape.