The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light distribution suggests a centrally dominant bulge component with a gradual decline in surface brightness outwards. The shape is primarily elliptical but not perfectly round, appearing slightly elongated. There are no strong indications of distinct spiral arms or a prominent disk structure. No significant tidal features or signs of major ongoing mergers are readily apparent. There is an intermediate to low rate of star formation occuring. The color profile suggests an older stellar population, consistent with a evolved galaxy.
