The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central bulge which emits stronger light than the surrounding regions. There appears to be a very faint hint of a disk structure with some slight features, but that is uncertain based on image quality. The color profile indicates a bias towards redder hues, suggesting an older stellar population and comparatively low ongoing star formation. There is no immediately apparent evidence of tidal disturbances or ongoing mergers in this image, however the galaxy is at a distance, which limits clear morphological observations. The galaxy exhibits a smooth light profile, suggesting a lack of prominent dust lanes.
