The galaxy presents a primarily smooth morphology, characterized by a dominant central bulge that appears approximately round. The light distribution indicates a generally well-mixed stellar population, although there is some evidence of a distinct, potentially reddened region to one side of the bulge. This region exhibits a more irregular shape and color, suggesting either a separate, smaller structure interacting with the primary galaxy or an area of ongoing or recent star formation heavily obscured by dust. No prominent spiral arm structures or other disk-like features are discernible in this image. The overall visual impression is that of a relatively quiescent galaxy with some possible disturbances or localized activity. The absolute magnitude indicates this is quite a luminous galaxy, and with the redshift being what it is, one could expect the galaxy to be reasonably large as well.
