The galaxy presents as an elliptical morphology. The central region exhibits a concentrated, bright core, transitioning into a diffuse halo. The light distribution appears smooth and centrally concentrated, indicating a likely older stellar population. The galaxy exhibits a slight elongation, it's shape leans more towards elliptical, it is neither perfectly circular nor highly elongated. There is no obvious presence of spiral arms or significant dust lanes, with no signs of active star formation. The galaxy displays a smooth, undisturbed structure, with no apparent signs of major tidal interactions or recent mergers. The color profile suggests a relatively red and quiescent system.
