The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. The shape is generally round. No spiral arms or obvious disk features are visible. The galaxy displays a yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. There is no indication of significant dust lanes or tidal features indicating recent or ongoing major merger activity, though subtle minor disturbances cannot be ruled out. The galaxy appears relatively isolated.
