The galaxy presents a predominantly smooth, elliptical morphology. It is characterized by a concentrated, bright central bulge that graduates outward into a fainter halo. There is little discernible disk structure or spiral arm features. The light distribution appears relatively symmetrical, with no obvious signs of major ongoing mergers or significant tidal disturbances. The galaxy exhibits a color profile consistent with an older stellar population. It appears as a somewhat yellow/orange hue, which is indicative of a population dominated by evolved stars and relatively low current star formation.
