The galaxy appears as a centrally concentrated object with a largely smooth morphology. There is a notable absence of well-defined spiral arms or a distinct disk structure. The light distribution suggests an elliptical or lenticular galaxy, characterized by a spheroid shape. The core region exhibits a high degree of luminosity, fading gradually towards the outer regions.

There may be some color variation within the galaxy, but the resolution limits any further morphological details. The overall color index indicates intermediate-aged stars within the galaxy, hinting at ongoing, but not extremely rapid, star formation. There are no signs of recent major mergers or tidal disturbances based on the smoothness of the galactic structure. Any potential minor irregularities may be masked by the distance and image resolution.
