The galaxy presents as a somewhat elliptical form, appearing moderately smooth with a hint of a disk-like structure. The central region is brighter and yellower, suggesting an older stellar population concentrated towards the core. Some subtle disturbances or features can be seen extending from the main body, indicating a possible interaction or recent merger event. The galaxy is not perfectly rounded but more intermediate, with a slight elongation along one axis. There is no clear evidence of strong spiral arms or bar structures.
