The galaxy presents a generally elliptical morphology, appearing somewhat elongated. The light profile indicates a dominant, smooth component, with a noticeable concentration of light towards the center. A faint, extended halo may be present, though it's poorly defined. There is some visual evidence of a possible disk-like structure.

Color gradients suggest a redder core and bluer outer regions. This could indicate an older stellar population in the center and younger stars towards the periphery. There seems to be some interaction with another galaxy in the image, however the galaxy is not significantly disturbed. The size of the galaxy seems small compared to other galaxies in the observable universe. The estimated stellar mass of the galaxy is relatively large.
