The galaxy presents as a centrally concentrated system with a relatively smooth morphology. The light profile appears diffuse, with a noticeable lack of distinct spiral arm structures or a prominent central bar. The overall shape is close to circular, showing a minor degree of ellipticity. There may be a faint tidal stream on one side of the galaxy; otherwise, there is no strong evidence for ongoing major merger activity or significant external disturbances. The galaxy exhibits a yellowish color, suggesting a population of older stars. 
