The galaxy presents as a relatively face-on lenticular type, exhibiting a bright, elliptical bulge which dominates its overall morphology. The bulge displays a smooth, concentrated luminosity profile, suggesting a relatively old stellar population. A faint, flattened disk surrounds the bulge, oriented along a major axis. The disk appears to be composed of older stars and lacks prominent spiral arm structures. Overall, the galaxy exhibits a smooth appearance with minimal visible dust lanes or star-forming regions. The galaxy's color is generally yellow/red, indicative of evolved stars with low levels of ongoing star formation. The estimated mass of the galaxy is substantial. Based on the Galaxy Zoo data it has been suggested that the galaxy might have undergone a merger event.
