The galaxy presents as a moderately luminous, relatively compact system. It exhibits a primarily smooth morphology, with a dominant central bulge that appears nearly spheroidal. A faint, diffuse disk component is suspected, exhibiting a slight elongation. The color profile suggests a population dominated by older stars, though a subtle blue hue hints at ongoing or recent star formation activity within the system. No distinct spiral arms or bar structures are discernible. Minor disturbances in the outer regions are possible, and it cannot be completely ruled out that the galaxy is undergoing a minor interaction. 
