The galaxy presents as a lenticular or possibly a spiral galaxy viewed at a high inclination. It exhibits a smooth overall structure with a noticeable central bulge. The disk appears relatively uniform in color, showing a predominantly blue hue that suggests ongoing or recent star formation. The object's morphology tends more toward an elongated shape than a circular one, yet it lacks any obvious signs of major disturbances that would indicate a recent or ongoing major merger. There appears to be some slight irregularity in the outskirts of the galaxy, possibly indicative of minor interactions or internal processes. The estimated mass of the galaxy is considerable. Despite its blue color, the specific star formation rate is low, indicating a relatively quiescent state.
