The galaxy presents as a centrally concentrated, luminous structure. Its morphology is largely smooth, lacking prominent spiral arms or a distinct disk component. The light distribution appears relatively uniform across the visible extent of the galaxy, suggesting an elliptical or lenticular morphology. The color is somewhat red, indicating a population dominated by older stars. There is no indication of active star formation regions or significant dust lanes. The overall shape is close to circular. There may be slight disturbances indicating a recent, minor interaction.
