The galaxy presents as a moderately luminous, disk-like structure, viewed at an oblique angle. The core region exhibits a high degree of central concentration, appearing smooth and bright, potentially indicating the presence of an older stellar population or a supermassive black hole. The disk component shows a fairly even distribution of light, with a hint of bluer hues, especially in the outer edges. This suggests on-going star formation. The galaxy's ellipticity is fairly high, with some asymmetry in the disk structure that may result from tidal interactions or internal processes. The general morphology suggests a galaxy transitioning between a spiral and elliptical galaxy type. 
