The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades outwards, lacking distinct spiral arms or a prominent disk structure. The light distribution appears relatively uniform, with a high degree of central concentration, and a somewhat round shape. There is no clear evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears to be relatively quiescent in terms of star formation, showing a population dominated by older stars. The object's apparent size is consistent with an average galaxy dimension at its estimated redshift. The galaxy appears to be quite isolated in this field of view.
