The galaxy presents as an elliptical or lenticular type, characterized by a centrally concentrated brightness profile that diminishes gradually towards the outer regions. It exhibits a generally smooth texture, with the majority of its light concentrated in the center of the galaxy. The color gradient suggests an older stellar population dominating the composition of the galaxy. The overall morphology is largely undisturbed, without obvious signs of recent mergers or tidal interactions. The galaxy appears well-defined and relatively isolated in the observed field.
