The galaxy presents an overall elliptical morphology with a relatively smooth, featureless appearance. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The galaxy's color profile suggests a population of older stars, with a subtle shift towards bluer hues in the outer regions. There is no apparent dust lane or spiral arm structure visible in the image. The galaxy displays a generally round shape, with only minor deviations from perfect circularity, and no signs of any major disturbances or ongoing merging events.
