The galaxy presents as a somewhat face-on spiral, exhibiting a central bulge with an apparent yellow-white color, suggesting a population of older stars. The spiral arms are not distinctly defined but appear loosely wound and exhibit a bluish tint, potentially indicative of ongoing star formation. The overall shape appears elliptical, elongated horizontally, but the high central concentration suggests it is more of a lenticular galaxy. There are no obvious signs of a recent major merger or tidal disturbances, although some minor asymmetry in the outer regions cannot be entirely ruled out. The galaxy appears moderately bright, with a relatively smooth overall texture.
