The galaxy presents an elongated morphology, appearing as a slightly distorted disk viewed at an oblique angle. A luminous central bulge is evident, exhibiting a yellowish hue, suggesting an older stellar population. Emanating from the central bulge are faint spiral arm structures, one appearing more diffuse and blueish, possibly indicating active star formation regions. The overall structure is somewhat disturbed, hinting at a possible interaction or merger event in its past. There is a region that looks like it is experiencing minor disturbance. The relative smoothness of the galaxy's profile suggests it is a relatively evolved system.
