The galaxy presents as a relatively small, centrally concentrated object. Its overall morphology appears smooth, lacking any obvious spiral arms or bar-like structure. The color profile suggests a redder population of stars, implying a lack of active star formation. There are some minor disturbances possibly indicating a weak interaction, but this may also be due to noise. There are some minor irregularities in the form of small patches of brighter light that may indicate younger stars. There is no apparent dust lane.
