The galaxy presents a generally smooth and rounded morphology. Its color profile suggests a population of older stars, with a dominant yellowish-orange hue. The overall appearance lacks any prominent spiral arm structure or significant dust lanes. There is a slight ellipticity to the galaxy's shape, deviating somewhat from a perfectly circular form. No indications of major mergers or significant tidal disturbances are readily apparent. The galaxy appears relatively isolated, with no immediately interacting companions visible in the field.
