The galaxy presents as a relatively compact, lenticular or early-type spiral system. A slight disclike structure is apparent. The galaxy exhibits a redder hue, suggestive of an older stellar population and potentially a lower rate of ongoing star formation. There is evidence of a slight irregularity or disturbance in its morphology, possibly the result of a minor interaction or merger event. However, the main body of the galaxy appears relatively undisturbed. There are no clearly defined spiral arms or prominent star-forming regions are observed, and the galaxy presents a relatively smooth overall appearance.
