The galaxy presents as a relatively smooth, elliptical morphology. Its light is concentrated towards the center, forming a bright, compact core. A gradual decline in surface brightness is observed moving outward from the core, lacking any sharply defined edges. The color profile suggests a population dominated by older stars, indicated by the redder, yellowish hue. There is little evidence of spiral arm structure or significant dust lanes. Its overall shape appears slightly elongated rather than perfectly spherical. Minimal signs of tidal disturbances or recent merger events are present.
