The galaxy presents as a relatively smooth and centralized structure. Its overall shape is oblong, tending towards elliptical but with a hint of a flattened disk. The light distribution appears concentrated towards the center, gradually fading into the surrounding background. A slight bluer tint is observable, suggestive of a younger stellar population. There may be minor disturbances to the overall structure, or indications of past interactions; however, this is not definitively clear from the image. The galaxy does not show any signs of significant merging activity at this resolution, though subtle distortions may exist.
