The galaxy presents as an elliptical structure with a bright, concentrated central bulge exhibiting a yellowish-white hue. This core region is surrounded by a more diffuse, bluish-white halo. The halo transitions into a fainter, more extended outer region, gradually fading into the background.

The overall color profile suggests a relatively old stellar population, particularly within the bulge. There is a slight hint of possible disk features or spiral arms as observed by the slight green tint on the outer rim of the bulge, although the morphology is predominantly smooth, it is not perfect.

There are no visually prominent signs of ongoing major merging activity or significant tidal disturbances, though a hint of structural irregularities may suggest minor interactions or internal dynamics are present.
