The galaxy presents as a relatively smooth, elongated object. Its overall shape is reminiscent of a flattened ellipsoid, with a high degree of axial ratio. The central region exhibits a concentration of light, appearing yellowish. This suggests an older stellar population dominating the core. The outer regions show a bluer hue, which may indicate younger stars and ongoing star formation, though perhaps at a modest rate. There is no immediately obvious spiral structure or significant dust lane obscuration. Minor irregularities are suspected which may be minor disturbances within the galaxy but there is no clear indication of a major interaction or merger.
