The galaxy presents a largely smooth and elliptical morphology. There appears to be little to no discernible spiral arm structure or distinct features such as dust lanes. The galaxy's light is concentrated towards a bright central bulge, which suggests a higher density of older stellar populations. The color of the galaxy appears to be yellowish-white, hinting at an intermediate age for the stellar population and relatively low recent star formation activity. Overall, the galaxy seems well-defined, and the morphology does not show signs of any major ongoing merger activity or significant tidal disturbances.
