The galaxy presents as an elliptical morphology, appearing generally smooth with a slight elongation. The core exhibits a bright, concentrated luminosity. The color profile suggests an older stellar population, with a dominant yellow hue. Hints of bluer star formation regions are present peripherally, indicating possible ongoing, albeit limited, stellar genesis. No distinct spiral arm structures or prominent dust lanes are apparent. Minor disturbances may be present but are difficult to discern without higher resolution imagery. The overall impression is of a galaxy approaching quiescence, displaying a mostly smooth structure indicative of previous mergers and a diminishing star formation rate.
