The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. Its color profile indicates a dominant yellowish hue, suggesting a population of older stars. There is a slight elongation visible in the galaxy's shape, deviating marginally from a perfectly circular form. No distinct spiral arms or bar structures are discernible; the galaxy appears primarily spheroidal, with a smooth and even distribution of light across its body. There is no obvious indication of any ongoing major merging activity or significant tidal disturbances.
