The galaxy presents as a somewhat elongated, diffuse object, exhibiting a smooth morphology. There is a relatively featureless appearance, with no obvious spiral arm structures or dust lanes visible at this resolution. The color profile suggests a redder hue, potentially indicating an older stellar population and a lower rate of active star formation. Based on the overall light distribution, the galaxy appears to be dominated by a spheroidal component, which would be consistent with it being an elliptical or lenticular galaxy. There is a possibility that it is undergoing some minor gravitational interaction with neighboring objects.
