The galaxy presents a largely smooth, elliptical morphology. It appears as a single, concentrated object, with a bright, unresolved central bulge. The shape appears to be somewhere between round and slightly elongated, with a possible hint of a disk component. There is no readily apparent dust lane or spiral structure. The light distribution suggests a relatively old stellar population, with a smooth light profile indicative of lower star formation activity, and little signs of any recent merging activity or major disturbances. The central region exhibits a bluer hue relative to the rest of the galaxy, and the galaxy appears more luminous in the g-band than in the r or z bands.
