The galaxy appears as a single, centrally concentrated light source. Its overall morphology suggests an elliptical galaxy type, exhibiting a smooth, featureless structure with no visible spiral arms or significant dust lanes. The light is brightest at the center, with a gradual decrease in intensity towards the outer edges. The color profile is relatively uniform, with a yellow/orange hue indicating an older stellar population dominated by evolved stars. There is no evidence of ongoing major merging activity or significant tidal distortions; the galaxy appears relatively undisturbed.
