The galaxy presents as an elliptical-type system, appearing largely featureless and smooth in morphology. It exhibits a concentrated central bulge that fades into a more diffuse halo. The galaxy appears round with no strong disturbances or interactions with neighboring galaxies. Color indices suggest a population of older stars, with the light trending towards the redder end of the spectrum. The overall light distribution suggests a relatively quiescent system, with low star formation activity.
