This galaxy appears to be an elliptical galaxy with a relatively smooth morphology. The light distribution suggests an "in between" roundness, neither perfectly spherical nor highly elongated. There appears to be little to no evidence of spiral arm structures. The color profile suggests a relatively older stellar population, with light emission skewed towards the red end of the spectrum. There are no prominent dust lanes or regions of active star formation readily apparent. Additionally, there are no indications of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure.
