The galaxy presents a generally smooth, elliptical morphology. The light profile shows a centrally concentrated bulge region with a gradual decrease in luminosity towards the outer regions, suggesting a relatively high degree of radial symmetry. The galaxy's color is predominantly yellowish-orange, suggestive of an older stellar population dominated by evolved stars, with little evidence of substantial recent star formation, although the hints of green suggest a very small amount of active star formation is occurring. There are no distinct spiral arm structures or prominent dust lanes visible. The overall shape is close to round, with only minor deviations from perfect circularity. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. It is a galaxy of considerable mass, and its absolute magnitude is high.
