The galaxy presents a largely smooth, elliptical morphology. The light profile suggests a high degree of central concentration, with a bright, unresolved core. There are no discernible spiral arms or bar structures. The galaxy's color is generally yellowish-white, potentially indicating a stellar population dominated by older, less massive stars. There are hints of a slight color gradient, with the central region potentially exhibiting a slightly redder hue. The galaxy exhibits a high degree of rotational symmetry, with a nearly circular appearance. There is no evidence of any major tidal disturbances or ongoing mergers.
