The galaxy presents a relatively smooth and rounded morphology. It appears as a concentrated, singular object, lacking any prominent spiral arms or bar structures. The color profile suggests an older stellar population, with a dominant reddish hue, indicative of evolved stars. There is minimal evidence of ongoing, significant star formation. The lack of distinct features suggests it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. A slight asymmetry may be present, but it is not substantial enough to categorize it as a disturbed system, or a system undergoing any major merging activity.
