The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. There is a dominant, moderately sized central bulge that appears relatively bright and smooth, fading towards the outer regions. Clear spiral arm structures are visible, with two or three main arms extending from the core. The arms display a medium degree of winding, appearing neither tightly wound nor loosely flung. The color suggests active star formation, though this activity is not excessively pronounced. No bar structure is obviously visible, though a faint linear structure may exist. There are no obvious signs of major tidal disturbances or ongoing mergers; however, the galaxy has some level of disturbance.
