The galaxy presents as a luminous, centrally concentrated object with a diffuse, extended halo. The central region exhibits a bright, yellowish-white color, suggesting an older stellar population. The outer regions fade into a more bluish hue, possibly indicating regions of younger star formation. The galaxy’s overall morphology is somewhat disturbed, showing signs of possible tidal interactions or past mergers, with irregular shapes and faint extensions detectable. The light distribution is neither perfectly elliptical nor spiral, leaning towards an irregular form. Faint blue regions are scattered across the galactic body hinting at on-going star formation. Overall, it appears to be a galaxy undergoing interaction or exhibiting post-merger features.
