The galaxy presents as a somewhat irregular, elliptical shape, with a noticeable central bulge that appears brighter and more concentrated. Surrounding the bulge is a more diffuse, disk-like structure. Faint, bluish tinges are visible in the outer regions of the disk, suggesting the presence of younger, hotter stars and ongoing star formation. Evident disturbances throughout the galaxy possibly indicate a merger event or interaction with another galaxy, with asymmetric features in the outer regions further supporting this assessment. The relative smoothness and centralized light concentration suggest a galaxy that has undergone some degree of dynamical relaxation, though the disturbances indicate a more recent interaction.
