The galaxy presents as an elliptical structure with a smooth, diffuse appearance, indicating an older stellar population. The core exhibits a concentrated luminosity, with a color gradient shifting towards redder hues from the center outwards. The absence of distinct spiral arms or significant dust lanes suggests a lack of ongoing, large-scale star formation. The overall morphology leans towards a spheroid shape, though some slight elongation is discernible, possibly indicating an oblate spheroid. No signs of tidal disturbances or recent merger events are visible within the immediate vicinity.
