The galaxy presents as a relatively smooth, amorphous structure. The light is concentrated towards the center, indicating a possible bulge. There are two main color components. The primary color is a dominant blue hue, suggesting the presence of younger, hotter stars and potentially active star formation. A secondary, smaller region shows a reddish-orange tint, possibly indicating older stellar populations or dust obscuration within that area. While not perfectly spherical, the galaxy is more rounded in appearance than disk-like, though some subtle elongation cannot be ruled out. There are no clear indications of major mergers, but a slight asymmetry or minor disturbance in the light distribution might suggest possible past interactions or internal dynamic processes. Overall, the galaxy appears as a low-mass system.
