The galaxy exhibits a generally smooth morphology, appearing largely featureless upon visual inspection. It has a predominantly elliptical shape, though it is not perfectly circular. The light is centrally concentrated, forming a bright core. Diffuse light extends outwards from the core, diminishing gradually with distance. The color gradient suggests an aging stellar population, transitioning from slightly yellow in the central regions to a more muted blue in the outer halo. There is no obvious presence of spiral arms or a well-defined disk structure. No evidence of ongoing major merger events or significant tidal disturbances is apparent. The overall appearance suggests a relatively evolved system.
