The galaxy presents as a somewhat rounded, elliptical structure with a smooth, diffuse light distribution. There is a central bulge that appears bright and yellowish, suggesting an older stellar population. Fainter, bluer light can be discerned in the surrounding regions, possibly indicating some ongoing, albeit limited, star formation. No prominent spiral arms or bar structures are apparent. There is evidence of only minor disturbances to the overall structure. The galaxy is estimated to have a diameter of approximately 10 kpc.
