The galaxy presents as a roughly elliptical, smooth-featured object. The core is luminous, exhibiting a concentrated brightness gradient outwards. No distinct spiral arms or a well-defined disk structure are apparent. The overall color profile suggests a population dominated by older stars, likely with a relatively low ongoing star formation rate. There is no strong indication of tidal features or recent merger activity. The galaxy exhibits a somewhat circular morphology. The light distribution suggests a relatively relaxed structure.
