The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and rounded morphology. It displays a concentrated central bulge which is brighter in yellow light compared to the outer regions. The outskirts appear to fade smoothly into the background, exhibiting a slightly more diffuse structure. There is no obvious spiral arm structure and it lacks significant dust lanes or prominent star-forming regions. No signs of a significant ongoing merger, tidal tails, or strong gravitational disturbances are seen. The overall light distribution suggests a well-mixed population of older stars. It shows a slight red hue, indicative of a relatively low rate of star formation.
