The galaxy presents a generally smooth morphology. It exhibits a noticeable central bulge that appears somewhat spherical. The overall shape is elliptical but appears to be close to the border between a mostly round shape and a somewhat elongated shape. A faint disk may be present, but the structure is not clearly defined, blending into the smooth appearance of the galaxy. The image shows some evidence of minor disturbances, which could indicate a past or ongoing interaction. There are no clear signs of a recent major merger. The color gradient suggests a population of older stars, particularly concentrated in the central bulge. This is also reflected in the relatively red color of the bulge. The rest of the galaxy is somewhat blue.
