The galaxy exhibits a moderately inclined spiral structure, appearing as a diffuse, slightly elongated luminous region. A central bulge is visible, contributing significantly to the overall luminosity, with an elliptical shape. The spiral arms are loosely wound and somewhat indistinct, showing a patchy distribution of light and color. There is a suggestion of some disturbance in the spiral arms, with a hint of merging activity or interaction. The galaxy is surrounded by a fainter, extended halo.
