The galaxy appears to be an elliptical type, exhibiting a centrally concentrated luminosity profile. The core region displays a bright, diffuse glow. Moving outward, the light intensity gradually diminishes, resulting in a smooth transition toward the galaxy's outer edges. The galaxy has an apparent shape that is slightly elongated, but remains generally rounded. There may be some minor irregularities or disturbances present within the galactic structure. There are no distinct spiral arm structures observed in the galaxy. There is no bright, compact nucleus, but the light of the galaxy concentrates towards the center of the galaxy. 
