The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The overall color appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue. There is little evidence of distinct spiral arms or dust lanes, and the galaxy's morphology suggests a system that is not highly disturbed. The galaxy appears to be roughly 4 kpc in radius. Given its color and form, star formation is likely low within the galaxy.
