The galaxy presents a generally smooth and elliptical morphology. A dominant central bulge is observed, exhibiting a yellowish-orange hue indicative of an older stellar population. The galaxy appears fairly regular and is well-defined. There is no apparent bar structure, and the spiral arms are either non-existent or very tightly wound, which is difficult to determine from the image. There is no notable asymmetry in the distribution of light. There are no visible signs of a recent major merger event.
