The galaxy presents as a relatively smooth, lens-shaped structure, with a bright, concentrated central bulge. It is observed at a significant inclination, providing a clear view of its disk. The disk component exhibits a flattened morphology. There is an apparent dust lane visible along the periphery of the galaxy. The overall color profile is primarily in the warmer spectrum, indicating a generally older stellar population and suppressed star formation. There are no prominent spiral arms or other significant features indicative of recent major mergers or active star formation. The morphology suggests a classification towards the S0, or lenticular, type.
