The galaxy presents as a single, luminous entity with a largely smooth morphology. The color profile suggests a population of older stars with relatively little active star formation. Its overall shape is approximately circular, exhibiting a high degree of symmetry with only the slightest deviation from perfect roundness, if any. No obvious spiral arms or bar structures are apparent. The galaxy lacks any readily discernible tidal features or signs of ongoing major mergers or interactions, although minor disturbances cannot be entirely ruled out. There may be some possible merger activity, but it is difficult to say for sure. 
