The galaxy presents a smooth, elliptical morphology with a highly concentrated central bulge. The galaxy exhibits a notable lack of distinct features such as spiral arms or prominent dust lanes. Its overall shape appears more elongated than circular, trending towards an intermediate ellipticity. There is no visible evidence of ongoing mergers or significant tidal disturbances affecting its structure. The color profile suggests a mature stellar population. Any star forming regions are likely minimal based on the color and lack of distinguishable structures.
