The galaxy presents as a slightly elongated object, exhibiting a central bulge that appears relatively smooth and moderately bright. The color profile suggests a bluish hue throughout the galaxy, indicating the presence of younger stellar populations, particularly in the disk. A subtle disk component is visible, though not distinctly defined. Indications of minor disturbances are present, with slight asymmetries in the galactic structure. There may be signs of possible faint tidal tails, and overall, the galaxy seems to be in a relatively undisturbed state, without major mergers or interactions.
