The galaxy presents a largely elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region is luminous, appearing a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the luminosity gradually decreases with a slight extension along one axis, indicating it is not perfectly spherical. There is minimal evidence of spiral arm structures or significant dust lanes within the galaxy. The lack of distinct features suggest a relatively quiescent state with low ongoing star formation. Some subtle irregularities in the outer halo may indicate past interactions or minor disturbances. Overall, it appears to be a massive, evolved galaxy with a relatively smooth structure.
