The galaxy presents as a somewhat elliptical structure, potentially categorized as an early-type spiral galaxy. It exhibits a bright, concentrated central bulge characterized by a yellowish-white hue, suggestive of an older stellar population and diminished star formation activity in this region. Diffuse, bluer patches extend from the central region. These likely correspond to regions of more recent star formation. The disk appears somewhat disturbed, possibly indicating an interaction or merger in the past. The galaxy appears quite massive.
