The galaxy presents an overall elliptical morphology, appearing relatively smooth and featureless. It exhibits a concentrated central bulge, emitting primarily in the redder wavelengths, suggesting an older stellar population dominates the core. The galaxy's color profile transitions towards bluer hues in the outer regions, indicating the presence of younger, star-forming regions away from the center, though these regions are not particularly pronounced or distinct. There are no observable spiral arms or bar structures. The galaxy shows little sign of significant tidal disturbances or ongoing mergers, maintaining a generally undisturbed appearance.
